DOCSLIB.ORG

Year Book 95.Pdf

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text

Load more

YEAR BOOK 95 The President's Report July 1,1995-June 30, 1996 • CARNEGIE INSTITUTION OF WASHINGTON • OFFICE OF ADMINISTRATION 1530 P Street, N.W. Washington, DC 20005-1910 (202) 387-6400 President: Maxine F. Singer Director, Administration and Finance: John]. Lively Director, External Affairs: Susanne Garvey DEPARTMENT OF EMBRYOLOGY 115 West University Parkway Baltimore, MD 21210-3301 (410) 554-1200 Director: Allan C. Spradlmg DEPARTMENT OF PLANT BIOLOGY 290 Panama Street Stanford, CA 943054101 (415) 325-1521 Director: Christopher Somervilk GEOPHYSICAL LABORATORY 5251 Broad Branch Road, N.W. Washington, DC 20015-1305 (202) 686-2410 Director: Charles T. Prewitt DEPARTMENT OF TERRESTRIAL MAGNETISM 5241 Broad Branch Road, N.W. Washington, DC 20015-1305 (202) 686-4370 Director: Sean C. Solomon THE OBSERVATORIES LAS CAMPANAS OBSERVATORY 813 Santa Barbara Street Casilla 601 Pasadena, CA 911014292 La Serena, Chile (818) 5774122 Director: Augustus Oemfcr, Jr., The Crawford H. Greenewak Chair Director, Las Campanas: Miguel Roth Carnegie Institution Web site; http://www.ciw.edu Library of" Congress Catalog Card Number 346716 ISSN CCW-OttoX; ISBN 0^727^6744 Printing by KirK Litfv^nifliic Company, Inc. Comp»*Mtu*n vuth AJrhe PageMaker Pecemkr \Wfr Contents Presidents Commentary (Singer) 1 Losses, Gains, Honors 10 Contributions, Gifts, and Private Grants 15 • The Observatories Director's Introduction 21 The Sky at Meter Wavelengths (McCarthy) 23 Lurking Galaxies (Dalcanton) 31 Personnel 37 Bibliography 39 • Department of Terrestrial Magnetism Director's Introduction 47 Time Scales and Stellar Evolution (Graham) 50 Star Dust in the Laboratory (Alexander) 57 Personnel 65 Bibliography 67 • Department of Embryology Director's Introduction 73 Mice Flip Over New Genetic Techniques (Dyrnecki) 77 Modem Genetics: A Modular Mis-expression Screen in. Drosophik (R0rth) . 82 Personnel 89 Bibliography 91 (continued) Yi \H fix 'K ^5 • C'\K\I i Al hoTHVIk >\ • Department of Plant Biology Director's Introduction 95 How Plants Protect Themselves from Damage by Excessive Sunlight (Niyogi, Grossman, and Bjorkman) 99 The Changing Carbon Cycle, from the Leaf to the Globe (Field) .. 106 Personnel 113 Bibliography 115 • Geophysical Laboratory Director's Introduction 119 Isotopic Tracers of Climatic Changes in the Australian Outback (Fogel and Johnson) 121 Ancient Structures: Probing the Chemistry of Organic Matter Diagenesis (Cody) 128 Ultrahigh Metamorphism and the Qinglongshan Anomaly (Rumble) 137 Personnel 140 Bibliography 142 Extradepartmental and Administrative Personnel 149 Publications and Special Events 150 Abstract of Minutes of the 104th Meeting of the Board 151 Bylaws 153 Financial Statements .. •, 162 Index. 175 C?me#ie Institution of Washing >n is committed to the national policy of fair treatment of all employees in .ill aspects of employment. The Institution Joes not discriminate against any person on the kw» at race, color, religion, HJX, national or ethnic origin, age, disability, veteran status, or .my other baai* prohjhiteJ h\ applicable law. This pt^licy ctwers all pri>grams, including adminis- trirti»*n ii ifA eJuc.1tion.4l pioftjram, aJmiK^nm ot qualified student!* as fellows, and empltfyment j d President and Trustees PRESIDENT Maxine E Singer BOARD OF TRUSTEES Thomas N. Urban, Chairman William I. M. Turner, Jr., Vice-Chairman William T. Golden, Secretary Philip H. Abelson William R. Hearst III William T. Coleman, jr. Richard E. Heckert John E Crawford Kazuo Inamori Edward E. David, Jr. Gerald D. Laubach John Diebold John D. Macomber James D. Ebert Richard A. Meserve W. Gary Ernst Frank Press Sandra M. Faber William J. Rutter Bruce W. Ferguson David E Swensen Michael E. Gellert Charles HL Townes Robert G. Goelet Sidney J. Weinberg, Jr. David Greenewalt TRUSTEES EMERITI Caryl P. Haskins William R. Hewlett William McChesney Martin, Jr. Richard S. Perkins Robert C. Seamans, Jr. Frank Stanton YHAR Fk vi; ^5 • C • Former Presidents and Trustees • PRESIDENTS Frederick H. Gillett, 1924-1935 Paul F. Oreffice, 1988-1993 Daniel C. Gilman, 1902-1908 William Church Osborn, 1927- Daniel Coit Gilman, 1902-1904 HannaH. Gray, 1974-1978 1934 Robert S. Woodward, 1904-1920 Crawford H. Greenewalt, 1952- Walter H. Page, 1971-1979 John C. Merriam, 1921-1938 1984 James Parmelee, 1917-1931 Vannevar Bush, 1939-1955 William C. Greenough, 1975- William Barclay Parsons, 1907- Caryl P. Haskins, 1956-1971 1989 1932 Philip H. Abelson, 1971-1978 Patrick E. Haggerty, 1974-1975 Stewart Paton, 1916-1942 James D. Ebert, 1978-1987 John Hay, 1902-1905 Robert N. Pennoyer, 1968-1989 Edward E. David, Jr. (Acting Barklie McKee Henry, 1949-1966 George W. Pepper, 1914-1919 President, 1987-1988) Myron T. Herrick, 1915-1929 John J. Pershing, 1930-1943 Abram S. Hewitt, 1902-1903 Henning W. Prentis, Jr., 1942- TRUSTEES Henry L. Higginson, 1902-1919 1959 Ethan A. Hitchcock, 1902-1909 Henry S. Pritchett, 1906-1936 Alexander Aggasiz, 1904-1905 Henry Hitchcock, 1902 Gordon S. Rentschler, 1946-1948 Robert O. Anderson, 1976-1983 Herbert Hoover, 1920-1949 Sally K. Ride, 1989-1994 Lord Ashby of Brandon, 1967- William Wirt Howe, 1903-1909 David Rockefeller, 1952-1956 1974 Charles L. Hutchinson, 1902- ElihuRoot, 1902-1937 J. Paul Austin, 1976-1978 1904 ElihuRoot, Jr., 1937-1967 George G. Baldwin, 1925-1927 Walter A. Jessup, 1938-1944 Julius Rosenwald, 1929-1931 Thomas Barbour, 1934-1946 Frank B. Jewett, 1933-1949 William M. Roth, 1968-1979 James F. Bell, 1935-1961 George F. Jewett, Jr., 1983-1987 William W. Rubey, 1962-1974 John S. Billings, 1902-1913 Antonia Ax:son Johnson, 1980- Martin A. Ryerson,-1908-1928 Robert Woods Bliss, 1936-1962 1994 Howard A. Schneiderman, 1988- Amory H. Bradford, 1959-1972 William F. Kieschnick, 1985-1991 1990 Lindsay Bradford, 1940-1958 Samuel P. Langley, 1904-1906 Henry R. Shepley, 1937-1962 Omar N. Bradley, 1948-1969 Kenneth G. Langone, 1993-1994 Theobald Smith, 1914-1934 Lewis M. Branscomb, 1973-1990 Ernest O. Lawrence, 1944-1958 JohnC. Spooner, 1902-1907 Robert S. Brookings, 1910-1929 Charles A. Lindbergh, 1934-1939 William Benson Storey, 1924- James E. Burke, 1989-1993 William Lindsay, 1902-1909 1939 Vannevar Bush, 1958-1971 Henry Cabot Lodge, 1914-1924 Richard P. Strong, 1934-1948 John L. Cadwalader, 1903-1914 Alfred L. Loomis, 1934-1973 Charles P. Taft, 1936-1975 William W. Campbell, 1929-1938 Robert A. Lovett, 1948-1971 William H. Taft, 1906-1915 John J. Carty, 1916-1932 SethLow, 1902-1916 William S. Thayer, 1929-1932 Whitefoord R. Cole, 1925-1934 Wayne MacVeagh, 1902-1907 JuanT. Trippe, 1944-1981 John T. Connor, 1975-1980 Keith S. McHugh, 1950-1974 James W. Wadsworth, 1932-1952 Frederic A. Delano, 1927-1949 Andrew W. Mellon, 1924-1937 Charles D. Walcott, 1902-1927 Cleveland H. Dodge, 1903-1923 JohnC. Merriam, 1921-1938 Frederic C. Walcott, 1931-1948 William E. Dodge, 1902-1903 J. lrwin Miller, 1988-1991 Henry P. Walcott, 1910-1924 Gerald M. Edelman, 1980-1987 Margaret Carnegie Miller, 1955— Lewis H. Weed, 1935-1952 Charles P. Fenner, 1914-1924 1967 William H. Welch, 1906-1934 Michael Ference, Jr., 1968-1980 Roswell Miller, 1933-1955 Gunnar Wessman, 1984-1987 Homer L. Ferguson, 1927-1952 Darius O. Mills, 1902-1909 Andrew D. White, 1902-1916 Simon Flexner, 1910-1914 S. Weir Mitchell, 1902-1914 Edward D. White, 1902-1903 W. Cameron Forbes, 1920-1955 Andrew J. Montague, 1907-1935 Henry White, 1913-1927 James Forrestal, 1948-1949 Henry S. Morgan, 1936-1978 James N. White, 1956-1979 William N. Frew, 1902-1915 William W. Morrow, 1902-1929 George W. Wickersham, 1909- Lyman J. Gage. 1902-1912 Seeley G. Mudd, 1940-1968 1936 Walter S. Giftbrd. 1931-1966 Franklin D. Murphy, 1978-1985 Robert E. Wilson, 1953-1964 Carl J. Gilbert, 1962-1983 William I. Myers, 1948-1976 Robert S. Woodward, 1905-1924 Cass Gilbert, 1924-1934 Garrison Norton, 1960-1974 Carroll D. Wright, 1902-1908 (: \: M , ni I win •:;<, \ • YEAR BOOK 95 Department of Terrestrial Magnetism staff member Erik Hauri and visitor Vincent Salters from Florida State University with the Cameca IMS 6f ion microprobe at DTM. The instrument, which enables researchers to examine micro-scale variations in trace elements and isotopes by bombarding samples with beams of charged particles, is run as a regional facility, with approximately half the operating time reserved for scientists from other institutions. It was formally dedicated in June 1996. (Photo by Steve Shirey) • V! hese are times of growing apprehension about how deeply the United States and several European countries are committed to the Tsupport of scientific research. Because the Carnegie Institution of Washington depends largely on an endowment for its annual operating funds, we feel less threatened by diminishing federal grants than other institutions. This circumstance is the consequence of decisions made decades ago by our trustees to eschew expansion on the basis of "soft" money. In exchange for our scientific independence, we have been somewhat limited in the scope and size of our research efforts. Consequently, our scientists have more freedom than many others to pursue long-term projects and risky new directions. We see our own earth filled n ., , . , * Besides being more indepen- with abundance, hut we forget . , ^ dent in research, Carnegie scien- to consider how much of that 11** i tists are relatively free from the abundance is owing to the scientific knowledge the vast academic resP^sibllities that machinery of the universe has burden their Peers in research unfolded* universities. They have no formal requirements for teaching. The Thomas Paine The Age of Reason, Part I substantial time and effort they 1794* .____^^ invest in graduate students and postdoctoral fellows rather reflect their recognition that teaching and research are interdependent endeavors. Committee work at Carnegie is generally rare and short-lived, unlike the time- consuming institutional committees that university faculty experience. These considerations suggest an idyllic world in which Carnegie staff scientists can devote themselves entirely to thinking important thoughts and doing ground- breaking experiments.
Recommended publications
  • II Publications, Presentations

    II Publications, Presentations

    II Publications, Presentations 1. Refereed Publications Izumi, K., Kotake, K., Nakamura, K., Nishida, E., Obuchi, Y., Ohishi, N., Okada, N., Suzuki, R., Takahashi, R., Torii, Abadie, J., et al. including Hayama, K., Kawamura, S.: 2010, Y., Ueda, A., Yamazaki, T.: 2010, DECIGO and DECIGO Search for Gravitational-wave Inspiral Signals Associated with pathfinder, Class. Quantum Grav., 27, 084010. Short Gamma-ray Bursts During LIGO's Fifth and Virgo's First Aoki, K.: 2010, Broad Balmer-Line Absorption in SDSS Science Run, ApJ, 715, 1453-1461. J172341.10+555340.5, PASJ, 62, 1333. Abadie, J., et al. including Hayama, K., Kawamura, S.: 2010, All- Aoki, K., Oyabu, S., Dunn, J. P., Arav, N., Edmonds, D., Korista sky search for gravitational-wave bursts in the first joint LIGO- K. T., Matsuhara, H., Toba, Y.: 2011, Outflow in Overlooked GEO-Virgo run, Phys. Rev. D, 81, 102001. Luminous Quasar: Subaru Observations of AKARI J1757+5907, Abadie, J., et al. including Hayama, K., Kawamura, S.: 2010, PASJ, 63, S457. Search for gravitational waves from compact binary coalescence Aoki, W., Beers, T. C., Honda, S., Carollo, D.: 2010, Extreme in LIGO and Virgo data from S5 and VSR1, Phys. Rev. D, 82, Enhancements of r-process Elements in the Cool Metal-poor 102001. Main-sequence Star SDSS J2357-0052, ApJ, 723, L201-L206. Abadie, J., et al. including Hayama, K., Kawamura, S.: 2010, Arai, A., et al. including Yamashita, T., Okita, K., Yanagisawa, TOPICAL REVIEW: Predictions for the rates of compact K.: 2010, Optical and Near-Infrared Photometry of Nova V2362 binary coalescences observable by ground-based gravitational- Cyg: Rebrightening Event and Dust Formation, PASJ, 62, wave detectors, Class.
  • Arxiv:2103.07476V1 [Astro-Ph.GA] 12 Mar 2021

    Arxiv:2103.07476V1 [Astro-Ph.GA] 12 Mar 2021

    FERMILAB-PUB-21-075-AE-LDRD Draft version September 3, 2021 Typeset using LATEX twocolumn style in AASTeX63 The DECam Local Volume Exploration Survey: Overview and First Data Release A. Drlica-Wagner ,1, 2, 3 J. L. Carlin ,4 D. L. Nidever ,5, 6 P. S. Ferguson ,7, 8 N. Kuropatkin ,1 M. Adamow´ ,9, 10 W. Cerny ,2, 3 Y. Choi ,11 J. H. Esteves,12 C. E. Mart´ınez-Vazquez´ ,13 S. Mau ,14, 15 A. E. Miller,16, 17 B. Mutlu-Pakdil ,2, 3 E. H. Neilsen ,1 K. A. G. Olsen ,6 A. B. Pace ,18 A. H. Riley ,7, 8 J. D. Sakowska ,19 D. J. Sand ,20 L. Santana-Silva ,21 E. J. Tollerud ,11 D. L. Tucker ,1 A. K. Vivas ,13 E. Zaborowski,2 A. Zenteno ,13 T. M. C. Abbott ,13 S. Allam ,1 K. Bechtol ,22, 23 C. P. M. Bell ,16 E. F. Bell ,24 P. Bilaji,2, 3 C. R. Bom ,25 J. A. Carballo-Bello ,26 D. Crnojevic´ ,27 M.-R. L. Cioni ,16 A. Diaz-Ocampo,28 T. J. L. de Boer ,29 D. Erkal ,19 R. A. Gruendl ,30, 31 D. Hernandez-Lang,32, 13, 33 A. K. Hughes,20 D. J. James ,34 L. C. Johnson ,35 T. S. Li ,36, 37, 38 Y.-Y. Mao ,39, 38 D. Mart´ınez-Delgado ,40 P. Massana,19, 41 M. McNanna ,22 R. Morgan ,22 E. O. Nadler ,14, 15 N. E. D. Noel¨ ,19 A. Palmese ,1, 2 A. H. G. Peter ,42 E. S.
  • Structural Analysis of the Sextans Dwarf Spheroidal Galaxy

    Structural Analysis of the Sextans Dwarf Spheroidal Galaxy

    MNRAS 000,1{16 (2015) Preprint 9 October 2018 Compiled using MNRAS LATEX style file v3.0 Structural analysis of the Sextans dwarf spheroidal galaxy T. A. Roderick,1? H. Jerjen,1 G. S. Da Costa,1 A. D. Mackey1 1Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia Accepted XXX. Received YYY; in original form ZZZ ABSTRACT We present wide-field g and i band stellar photometry of the Sextans dwarf spheroidal galaxy and its surrounding area out to four times its half-light radius (rh = 695 pc), based on images obtained with the Dark Energy Camera at the 4-m Blanco tele- scope at CTIO. We find clear evidence of stellar substructure associated with the galaxy, extending to a distance of 820 (2 kpc) from its centre. We perform a sta- tistical analysis of the over-densities and find three distinct features, as well as an extended halo-like structure, to be significant at the 99:7% confidence level or higher. Unlike the extremely elongated and extended substructures surrounding the Hercules dwarf spheroidal galaxy, the over-densities seen around Sextans are distributed evenly about its centre, and do not appear to form noticeable tidal tails. Fitting a King 0 0 model to the radial distribution of Sextans stars yields a tidal radius rt = 83:2 ± 7:1 (2.08±0.18 kpc), which implies the majority of detected substructure is gravitationally bound to the galaxy. This finding suggests that Sextans is not undergoing significant tidal disruption from the Milky Way, supporting the scenario in which the orbit of Sextans has a low eccentricity.
  • Dark Matter Searches Targeting Dwarf Spheroidal Galaxies with the Fermi Large Area Telescope

    Dark Matter Searches Targeting Dwarf Spheroidal Galaxies with the Fermi Large Area Telescope

    Doctoral Thesis in Physics Dark Matter searches targeting Dwarf Spheroidal Galaxies with the Fermi Large Area Telescope Maja Garde Lindholm Oskar Klein Centre for Cosmoparticle Physics and Cosmology, Particle Astrophysics and String Theory Department of Physics Stockholm University SE-106 91 Stockholm Stockholm, Sweden 2015 Cover image: Top left: Optical image of the Carina dwarf galaxy. Credit: ESO/G. Bono & CTIO. Top center: Optical image of the Fornax dwarf galaxy. Credit: ESO/Digitized Sky Survey 2. Top right: Optical image of the Sculptor dwarf galaxy. Credit:ESO/Digitized Sky Survey 2. Bottom images are corresponding count maps from the Fermi Large Area Tele- scope. Figures 1.1a, 1.2, 1.3, and 4.2 used with permission. ISBN 978-91-7649-224-6 (pp. i{xxii, 1{120) pp. i{xxii, 1{120 c Maja Garde Lindholm, 2015 Printed by Publit, Stockholm, Sweden, 2015. Typeset in pdfLATEX Abstract In this thesis I present our recent work on gamma-ray searches for dark matter with the Fermi Large Area Telescope (Fermi-LAT). We have tar- geted dwarf spheroidal galaxies since they are very dark matter dominated systems, and we have developed a novel joint likelihood method to com- bine the observations of a set of targets. In the first iteration of the joint likelihood analysis, 10 dwarf spheroidal galaxies are targeted and 2 years of Fermi-LAT data is analyzed. The re- sulting upper limits on the dark matter annihilation cross-section range 26 3 1 from about 10− cm s− for dark matter masses of 5 GeV to about 5 10 23 cm3 s 1 for dark matter masses of 1 TeV, depending on the × − − annihilation channel.
  • Model Comparison of the Dark Matter Profiles

    Model Comparison of the Dark Matter Profiles

    A&A 558, A35 (2013) Astronomy DOI: 10.1051/0004-6361/201321606 & c ESO 2013 Astrophysics Model comparison of the dark matter profiles of Fornax, Sculptor, Carina and Sextans Maarten A. Breddels and Amina Helmi Kapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, The Netherlands e-mail: [email protected] Received 28 March 2013 / Accepted 16 August 2013 ABSTRACT Aims. We compare dark matter profile models of four dwarf spheroidal galaxies satellites of the Milky Way using Bayesian evidence. Methods. We use orbit based dynamical models to fit the 2nd and 4th moments of the line of sight velocity distributions of the Fornax, Sculptor, Carina and Sextans dwarf spheroidal galaxies. We compare NFW, Einasto and several cored profiles for their dark halos and present the probability distribution functions of the model parameters. Results. For each galaxy separately we compare the evidence for the various dark matter profiles, and find that it is not possible to distinguish between these specific parametric dark matter density profiles using the current data. Nonetheless, from the combined 2 β/2 evidence, we find that is unlikely that all galaxies are embedded in the same type of cored profiles of the form ρDM ∝ 1/(1 + r ) , where β = 3, 4. For each galaxy, we also obtain an almost model independent, and therefore accurate, constraint on the logarithmic slope of the dark matter density distribution at a radius ∼r−3, i.e. where the logarithmic slope of the stellar density profile is −3. Conclusions. For each galaxy, we find that all best fit models essentially have the same mass distribution over a large range in radius (from just below r−3 to the last measured data point).
  • The Variable Star Population in the Sextans Dwarf Spheroidal Galaxy

    The Variable Star Population in the Sextans Dwarf Spheroidal Galaxy

    TheThe variablevariable starstar populationpopulation inin thethe SextansSextans dwarfdwarf spheroidalspheroidal galaxygalaxy Kathy Vivas Cerro Tololo Interamerican Observatory La Serena, Chile In collaboration with Javier Alonso-García (U. of Antofagasta, Chile) Mario Mateo (U. of Michigan, USA) Alistair Walker (CTIO, Chile) David Nidever (NOAO, USA) DECam Community Science Workshop 2018 1 The Role of Variable Stars ● Tracers of different stellar populations ● Standard candles → Distance Scale Variable stars in the Carina dwarf spheroidal galaxy (Vivas & Mateo 2013) DECam Community Science Workshop 2018 2 Properties of the Satellites of the Milky Way Drlica-Wagner et al., 2015 The new discoveries are likely to be ultra-faint dwarf galaxies. Gallart et al. 2015 Classical dwarfs display a variety of SFRs DECam Community Science Workshop 2018 3 CMDs of Satellite Dwarfs Brown et al 2014 On the other hand, ultra-faint dwarfs seem Monelli et al 2003 to be consistent with only and old Galaxies like Carina show obvious population signs of multiple bursts of star formation DECam Community Science Workshop 2018 4 Leo T: a UFD with extended star formation Clementini et al (2012) DECam Community Science Workshop 2018 5 Helium-Burning Pulsating Stars 3.0 Anomalous Cepheids 2.0 0.7 RR Lyrae Stars Variable stars and theoretical isochrones in Leo I (Fiorentino et al 2012) DECam Community Science Workshop 2018 6 Dwarf Cepheid Stars (collective name for δ Scuti or SX Phe) Intermediate age population TO Old Population TO Coppola et al 2015, Vivas & Mateo 2013 DECam Community Science Workshop 2018 7 Dwarf Cepheids as distance indicators Need to study more systems! Cohen et al (2012) P-L relationship (independent of metallicity) → standard candles DECam Community Science Workshop 2018 8 Dwarf Cepheids in other galaxies 85 dwarf cepheids in Fornax A few thousand in (Poretti et al.
  • On the Application of Stark Broadening Data Determined with a Semiclassical Perturbation Approach

    On the Application of Stark Broadening Data Determined with a Semiclassical Perturbation Approach

    Atoms 2014, 2, 357-377; doi:10.3390/atoms2030357 OPEN ACCESS atoms ISSN 2218-2004 www.mdpi.com/journal/atoms Article On the Application of Stark Broadening Data Determined with a Semiclassical Perturbation Approach Milan S. Dimitrijević 1,2,* and Sylvie Sahal-Bréchot 2 1 Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia 2 Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique, Observatoire de Paris, UMR CNRS 8112, UPMC, 5 Place Jules Janssen, 92195 Meudon Cedex, France; E-Mail: [email protected] (S.S.-B.) * Author to whom correspondence should be addressed; E-Mail: [email protected]; Tel.: +381-64-297-8021; Fax: +381-11-2419-553. Received: 5 May 2014; in revised form: 20 June 2014 / Accepted: 16 July 2014 / Published: 7 August 2014 Abstract: The significance of Stark broadening data for problems in astrophysics, physics, as well as for technological plasmas is discussed and applications of Stark broadening parameters calculated using a semiclassical perturbation method are analyzed. Keywords: Stark broadening; isolated lines; impact approximation 1. Introduction Stark broadening parameters of neutral atom and ion lines are of interest for a number of problems in astrophysical, laboratory, laser produced, fusion or technological plasma investigations. Especially the development of space astronomy has enabled the collection of a huge amount of spectroscopic data of all kinds of celestial objects within various spectral ranges. Consequently, the atomic data for trace elements, which had not been
  • First Detections of FS Canis Majoris Stars in Clusters Evolutionary State As Constrained by Coeval Massive Stars

    First Detections of FS Canis Majoris Stars in Clusters Evolutionary State As Constrained by Coeval Massive Stars

    A&A 575, A10 (2015) Astronomy DOI: 10.1051/0004-6361/201425371 & c ESO 2015 Astrophysics First detections of FS Canis Majoris stars in clusters Evolutionary state as constrained by coeval massive stars D. de la Fuente1, F. Najarro1,C.Trombley2,B.Davies3, and D. F. Figer2 1 Centro de Astrobiología (CSIC/INTA), ctra. de Ajalvir km. 4, 28850 Torrejón de Ardoz, Madrid, Spain e-mail: [email protected] 2 Center for Detectors, Rochester Institute of Technology, 74 Lomb Memorial Drive, Rochester, NY 14623, USA 3 Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool L3 5RF, UK Received 19 November 2014 / Accepted 23 December 2014 ABSTRACT Context. FS CMa stars are low-luminosity objects showing the B[e] phenomenon whose evolutionary state remains a puzzle. These stars are surrounded by compact disks of warm dust of unknown origin. Hitherto, membership of FS CMa stars to coeval populations has never been confirmed. Aims. The discovery of low-luminosity line emitters in the young massive clusters Mercer 20 and Mercer 70 prompts us to investigate the nature of such objects. We intend to confirm membership to coeval populations in order to characterize these emission-line stars through the cluster properties. Methods. BasedonISAAC/VLT medium-resolution spectroscopy and NICMOS/HST photometry of massive cluster members, new characterizations of Mercer 20 and Mercer 70 are performed. Coevality of each cluster and membership of the newly-discovered B[e] objects are investigated using our observations as well as literature data of the surroundings. Infrared excess and narrow-band photometric properties of the B[e] stars are also studied.
  • The Galaxies of the Local Group Sidney Van Den Bergh Frontmatter More Information

    The Galaxies of the Local Group Sidney Van Den Bergh Frontmatter More Information

    Cambridge University Press 978-0-521-03743-3 - The Galaxies of the Local Group Sidney van den Bergh Frontmatter More information The Local Group is a small cluster of galaxies of which 35 members are currently known, including the Milky Way. It is believed that at least half of all galaxies in the Universe belong to similar groups. Galaxies of the Local Group can be used as “stepping stones” to determine the distance to more remote galaxies, and thus they help to measure the size and age of the Universe. Studying stars of differing ages in different members of the Local Group allows us to see how galaxies evolve over timescales in excess of 10 billion years. The oldest stars in the Local Group galaxies also provide critical information on the physical conditions of the early Universe. The Local Group thus provides many valuable clues to understanding the rest of the Universe. This authoritative volume provides a comprehensive and up-to-date synthesis of what is currently known about the Local Group of galaxies. It includes a summary of our knowledge of each of the individual member galaxies, as well as those galaxies previously regarded as possible members. After examining each galaxy in detail, the book goes on to examine the mass, stability, and evolution of the Local Group as a whole. The book includes many important previously unpublished results and conclusions. With characteristic clarity, Professor van den Bergh provides in this book a mas- terful summary of all that is known about the galaxies of the Local Group and their evolution, and he expertly places this knowledge in the wider context of ongoing studies of galaxy formation and evolution, the cosmic distance scale, and the condi- tions in the early Universe.
  • First Detections of FS Canis Majoris Stars in Clusters. Evolutionary State

    First Detections of FS Canis Majoris Stars in Clusters. Evolutionary State

    Astronomy & Astrophysics manuscript no. paper1_v7 c ESO 2018 August 20, 2018 First detections of FS Canis Majoris stars in clusters Evolutionary state as constrained by coeval massive stars⋆ D. de la Fuente1, F. Najarro1, C. Trombley2, B. Davies3, and D. F. Figer2 1 Centro de Astrobiología (CSIC/INTA), ctra. de Ajalvir km. 4, 28850 Torrejón de Ardoz, Madrid, Spain e-mail: [email protected] 2 Center for Detectors, Rochester Institute of Technology, 74 Lomb Memorial Drive, Rochester, NY 14623, USA 3 Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool L3 5RF, UK Received 19 November 2014 / Accepted 23 december 2014 ABSTRACT Context. FS CMa stars are low-luminosity objects showing the B[e] phenomenon whose evolutionary state remains a puzzle. These stars are surrounded by compact disks of warm dust of unknown origin. Hitherto, membership of FS CMa stars to coeval populations has never been confirmed. Aims. The discovery of low-luminosity line emitters in the young massive clusters Mercer 20 and Mercer 70 prompts us to investigate the nature of such objects. We intend to confirm membership to coeval populations in order to characterize these emission-line stars through the cluster properties. Methods. Based on ISAAC/VLT medium-resolution spectroscopy and NICMOS/HST photometry of massive cluster members, new characterizations of Mercer 20 and Mercer 70 are performed. Coevality of each cluster and membership of the newly-discovered B[e] objects are investigated using our observations as well as literature data of the surroundings. Infrared excess and narrow-band photometric properties of the B[e] stars are also studied.
  • Biennial Report 2004 2005 Published in Spain by the ISAAC NEWTON GROUP of TELESCOPES (ING) ISSN 1575–8966 Legal License: TF–1142 /99

    Biennial Report 2004 2005 Published in Spain by the ISAAC NEWTON GROUP of TELESCOPES (ING) ISSN 1575–8966 Legal License: TF–1142 /99

    I SAAC N EWTON G ROUP OF T ELESCOPES Biennial Report 2004 2005 Published in Spain by the ISAAC NEWTON GROUP OF TELESCOPES (ING) ISSN 1575–8966 Legal license: TF–1142 /99 Apartado de correos, 321 E-38700 Santa Cruz de La Palma; Canary Islands; Spain Tel: +34 922 425 400 Fax: +34 922 425 401 URL: http://www.ing.iac.es/; http://www.ast.cam.ac.uk/ING/ (UK mirror) Editor and designer: Javier Méndez ([email protected]) Preprinting: Gráficas El Time. Tel: +34 922 416 651 Printing: Gráficas Sabater. Tel: +34 922 623 555 Front cover: IC1396 or the Elephant Trunk Nebula. Image obtained as part of the Isaac Newton Telescope Photometric Hα Survey of the Northen Galactic Plane, and it was prepared by Nick Wright, University College London. Inset: Photograph of laser test on the William Herschel Telescope as part of GLAS preparatory study. Credit: Javier Méndez. Other picture credits: Nik Szymanek (WHT, p. 4); Nik Szymanek (INT, p. 4); Nik Szymanek (JKT, p. 4); Nik Szymanek (ING, p. 5); Jens Moser (WHT, back); Jens Moser (INT, back); Nik Szymanek (JKT, back). The ING Biennial Report is available online at http://www.ing.iac.es/PR/AR/ or at http://www.ast.cam.ac.uk/ING/PR/AR/. ISAAC NEWTON GROUP OF TELESCOPES Biennial Report of the PPARC-NWO-IAC ING Board 2004 – 2005 ISAAC NEWTON GROUP William Herschel Telescope Isaac Newton Telescope Jacobus Kapteyn Telescope 4 • ING BIENNIAL R EPORT 2004–2005 OF TELESCOPES The Isaac Newton Group of Telescopes (ING) consists of the 4.2- metre William Herschel Telescope (WHT), the 2.5-metre Isaac Newton Telescope (INT) and the 1.0-metre Jacobus Kapteyn Telescope (JKT).
  • List of Publications (06/2021)

    List of Publications (06/2021)

    Prof. Dr. Eva K. Grebel, Astronomisches Rechen-Institut, Zentrum f¨urAstronomie der Universit¨at Heidelberg, M¨onchhofstr. 12{14, D-69120 Heidelberg, Germany List of Publications (06/2021) A. Refereed publications (443) . 1 B. Reviews (34) . 47 C. Conference proceedings etc. (175) 50 D. Abstracts (141) . 66 E. Books (2) . 77 In publications with my students or postdocs their names are underlined when this work was completed (or partially carried out) while they held their position with me. A. Refereed Publications 1. Menon, S.H., Grasha, K., Elmegreen, B.G., Federrath, C., Krumholz, M.R., Calzetti, D., S´anchez, N., Linden, S.T., Adamo, A., Messa, M., Cook, D.O., Dale, D.A., Grebel, E.K., Fumagalli, M., Sabbi, E., Johnson, K.E., Smith, L.J., & Kennicutt, R.C. The Dependence of the Hierarchical Distribution of Star Clusters on Galactic En- vironment 2021, MNRAS, submitted 2. D´ek´any, I., Grebel, E.K., & Pojmanski, G. Metallicity estimation of RR Lyrae stars from their I-band light curves 2021, ApJ, submitted 3. Gatto, M., Ripepi, V., Bellazzini, M., Tosi, M., Cignoni, M., Tortora, C., Leccia, S., Clementini, G., Grebel, E.K., Longo, G., Marconi, M., & Musella, I. STEP Survey II: Structural Analysis of 170 star clusters in the SMC 2021, MNRAS, submitted 4. Orozco-Duarte, R., Wofford, A., Vidal-Garc´ıa, A., Bruzual, G., Charlot, S., Krumholz, M., Hannon, S., Lee, J., Wofford, T., Fumagalli, M., Dale, D., Messa, M., Grebel, E.K., Smith, L., Grasha, K., & Cook, D. Synthetic photometry of OB star clusters with stochastically sampled IMFs: anal- ysis of models and HST observations 2021, MNRAS, submitted 5.