David K. Lynch, Phd
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
THE YOUNG ASTRONOMERS NEWSLETTER Volume 23 Number 6 STUDY + LEARN = POWER May 2015
THE YOUNG ASTRONOMERS NEWSLETTER Volume 23 Number 6 STUDY + LEARN = POWER May 2015 ****************************************************************************************************************************** AUSTRALIAN CRATER HIDDEN STARS A team of geophysicists has found the twin scars of Scientists found a bright nebula around the Milky the impacts of a huge meteorite that broke in two Way”s nearby star 48 Librae in a patch of sky that moments before it slammed into the Earth millions of appears totally black in visible light but appears in infra- years ago in central Australia. It is the largest impact red. They said: "This cluster is probably a group of very zone ever found on Earth – 400 kilometers wide. young stars forming inside a previously undiscovered “YELLOW BALLS” molecular cloud, and the 48 Librae nebula apparently is Citizen scientists recently found a new class of due to a huge cloud of dust around the star.” curiosities that had gone unrecognized before: yellow HUBBLE IS 25! balls. Many "citizen scientist" projects make up the Hubble, the first telescope to revolutionize modern Zooniverse website which relies on “crowd-sourcing” to astronomy and change our view of the universe by help process scientific data. offering glimpses of distant galaxies, has marked its 25th The rounded features are not actually yellow but year in space. A senior scientist said: "Hubble absolutely appear that way in the infrared images the telescope has changed the way humans look at the universe and sends to Earth. See: http://www.spxdaily.com/images- our place in it." lg/yellow-balls-process-star-formation-lg.jpg A DISTANT PLANET and http://www.zooniverse.org The Spitzer Space Telescope teamed up with CANADA’S NEW TMT TELESCOPE Poland’s OGLE telescope in Chile to find a remote gas Canada and an international partnership are funding planet about 13,000 light-years away, making it one of the construction of the Thirty Meter Telescope - the top the most distant planets known. -
UKRAINIAN FOOD JOURNAL 2016 V.5 Is.3.Pdf
ISSN 2313–5891 (Online) ISSN 2304–974X (Print) Ukrainian Food Journal Volume 5, Issue 3 2016 Kyiv Kиїв 2016 Ukrainian Food Journal is an Ukrainian Food Journal – міжнародне international scientific journal that наукове періодичне видання для publishes innovative papers of expert in the публікації результатів досліджень fields of food science, engineering and фахівців у галузі харчової науки, техніки technology, chemistry, economics and та технології, хімії, економіки і management. управління. The advantage of research results Перевага в публікації результатів publication available to students, graduate досліджень надається студентам, students, young scientists. аспірантам та молодим вченим. Ukrainian Food Journal is abstracted and Ukrainian Food Journal індексується indexed by scientometric databases: наукометричними базами: Index Copernicus (2012) EBSCO (2013) Google Scholar (2013) UlrichsWeb (2013) Global Impact Factor (2014) CABI full text (2014) Online Library of University of Southern Denmark (2014) Directory of Research Journals Indexing (DRJI) (2014) Universal Impact Factor (2014) Directory of Open Access scholarly Resources (ROAD) (2014) European Reference Index for the Humanities and the Social Sciences (ERIH PLUS) (2014) Directory of Open Access Journals (DOAJ) (2015) InfoBase Index (2015) Chemical Abstracts Service Source Index (CASSI) (2016) Ukrainian Food Journal включено у перелік наукових фахових видань України з технічних наук, в якому можуть публікуватися результати дисертаційних робіт на здобуття наукових ступенів доктора і кандидата наук (Наказ Міністерства освіти і науки України № 1609 від 21.11.2013) Editorial office address: Адреса редакції: National University Національний університет of Food Technologies харчових технологій Volodymyrska str., 68 вул. Володимирська, 68 Ukraine, Kyiv 01601 Київ 01601 e-mail: [email protected] Scientific Council of the National Рекомендовано вченою радою University of Food Technologies Національного університету recommends the journal for printing. -
Arxiv:1403.4250V2 [Astro-Ph.GA] 9 Jun 2014 Nelemans Et Al
Submitted to The Astrophysical Journal Preprint typeset using LATEX style emulateapj v. 5/2/11 CONSTRAINTS ON THE PROGENITOR SYSTEM OF THE TYPE IA SUPERNOVA 2014J FROM PRE-EXPLOSION HUBBLE SPACE TELESCOPE IMAGING Patrick L. Kelly1, Ori D. Fox1, Alexei V. Filippenko1, S. Bradley Cenko2, Lisa Prato3, Gail Schaefer4, Ken J. Shen1,5, WeiKang Zheng1, Melissa L. Graham1, and Brad E. Tucker1,6 Submitted to The Astrophysical Journal ABSTRACT We constrain the properties of the progenitor system of the highly reddened Type Ia supernova (SN) 2014J in Messier 82 (M82; d ≈ 3:5 Mpc). We determine the SN location using Keck-II K-band adaptive optics images, and we find no evidence for flux from a progenitor system in pre-explosion near-ultraviolet through near-infrared Hubble Space Telescope (HST) images. Our upper limits exclude systems having a bright red giant companion, including symbiotic novae with luminosities comparable to that of RS Ophiuchi. While the flux constraints are also inconsistent with predictions for compar- atively cool He-donor systems (T . 35,000 K), we cannot preclude a system similar to V445 Puppis. The progenitor constraints are robust across a wide range of RV and AV values, but significantly greater values than those inferred from the SN light curve and spectrum would yield proportionally brighter luminosity limits. The comparatively faint flux expected from a binary progenitor system consisting of white dwarf stars would not have been detected in the pre-explosion HST imaging. In- frared HST exposures yield more stringent constraints on the luminosities of very cool (T < 3000 K) companion stars than was possible in the case of SN Ia 2011fe. -
Thunderkat: the Meerkat Large Survey Project for Image-Plane Radio Transients
ThunderKAT: The MeerKAT Large Survey Project for Image-Plane Radio Transients Rob Fender1;2∗, Patrick Woudt2∗ E-mail: [email protected], [email protected] Richard Armstrong1;2, Paul Groot3, Vanessa McBride2;4, James Miller-Jones5, Kunal Mooley1, Ben Stappers6, Ralph Wijers7 Michael Bietenholz8;9, Sarah Blyth2, Markus Bottcher10, David Buckley4;11, Phil Charles1;12, Laura Chomiuk13, Deanne Coppejans14, Stéphane Corbel15;16, Mickael Coriat17, Frederic Daigne18, Erwin de Blok2, Heino Falcke3, Julien Girard15, Ian Heywood19, Assaf Horesh20, Jasper Horrell21, Peter Jonker3;22, Tana Joseph4, Atish Kamble23, Christian Knigge12, Elmar Körding3, Marissa Kotze4, Chryssa Kouveliotou24, Christine Lynch25, Tom Maccarone26, Pieter Meintjes27, Simone Migliari28, Tara Murphy25, Takahiro Nagayama29, Gijs Nelemans3, George Nicholson8, Tim O’Brien6, Alida Oodendaal27, Nadeem Oozeer21, Julian Osborne30, Miguel Perez-Torres31, Simon Ratcliffe21, Valerio Ribeiro32, Evert Rol6, Anthony Rushton1, Anna Scaife6, Matthew Schurch2, Greg Sivakoff33, Tim Staley1, Danny Steeghs34, Ian Stewart35, John Swinbank36, Kurt van der Heyden2, Alexander van der Horst24, Brian van Soelen27, Susanna Vergani37, Brian Warner2, Klaas Wiersema30 1 Astrophysics, Department of Physics, University of Oxford, UK 2 Department of Astronomy, University of Cape Town, South Africa 3 Department of Astrophysics, Radboud University, Nijmegen, the Netherlands 4 South African Astronomical Observatory, Cape Town, South Africa 5 ICRAR, Curtin University, Perth, Australia 6 University -
The Orbital Period of V458 Vulpeculae, a Post Double Common-Envelope Nova
Mon. Not. R. Astron. Soc. 000, 1–6 (2010) Printed 11 November 2018 (MN LATEX style file v2.2) The orbital period of V458 Vulpeculae, a post double common-envelope nova P. Rodr´ıguez-Gil1,2,3⋆, M. Santander-Garc´ıa1,2,3, C. Knigge4, R. L. M. Corradi2,3, B. T. G¨ansicke5, M. J. Barlow6, J. J. Drake7, J. Drew8, B. Miszalski8, R. Napiwotzki8, D. Steeghs5, R. Wesson6, A. A. Zijlstra9, D. Jones9, T. Liimets10,1, S. Pyrzas1,5 and M. M. Rubio-D´ıez1,11 1Isaac Newton Group of Telescopes, Apartado de Correos 321, Santa Cruz de La Palma, E-38700, Spain 2Instituto de Astrof´ısica de Canarias, V´ıa L´actea, s/n, La Laguna, E-38205, Santa Cruz de Tenerife, Spain 3Departamento de Astrof´ısica, Universidad de La Laguna, La Laguna, E-38205, Santa Cruz de Tenerife, Spain 4School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK 5Department of Physics, University of Warwick, Coventry CV4 7AL, UK 6Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK 7Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 8Centre for Astrophysics Research, STRI, University of Hertfordshire, College Lane Campus, Hatfield AL10 9AB, UK 9Jodrell Bank Center for Astrophysics, Alan Turing Building, The University of Manchester, Oxford Road, Manchester M13 9PL, UK 10Tartu Observatoorium, T˜oravere 61602, Estonia 11Centro de Astrobiolog´ıa (CSIC/INTA), Ctra. de Torrej´on a Ajalvir, km 4, E-28850 Torrej´on de Ardoz, Madrid, Spain Accepted 2010. Received 2010 ABSTRACT We present time-resolved optical spectroscopy of V458 Vulpeculae (Nova Vul 2007 No. -
Chemical-Composition-Of-The-Circumstellar-Disk-Around-AB-Aurigae.Pdf (1.034Mb)
Astronomy & Astrophysics manuscript no. AB_Aur_final c ESO 2015 May 12, 2015 Chemical composition of the circumstellar disk around AB Aurigae S. Pacheco-Vázquez1 , A. Fuente1, M. Agúndez2, C. Pinte6, 7, T. Alonso-Albi1, R. Neri3, J. Cernicharo2,J. R. Goicoechea2, O. Berné4, 5, L. Wiesenfeld6, R. Bachiller1, and B. Lefloch6 1 Observatorio Astronómico Nacional (OAN), Apdo 112, E-28803 Alcalá de Henares, Madrid, Spain e-mail: [email protected], [email protected] 2 Instituto de Ciencia de Materiales de Madrid, ICMM-CSIC, C/ Sor Juana Inés de la Cruz 3, E-28049 Cantoblanco, Spain e-mail: [email protected] 3 Institut de Radioastronomie Millimétrique, 300 Rue de la Piscine, F-38406 Saint Martin d’Hères, France 4 Université de Toulouse, UPS-OMP, IRAP, Toulouse, France 5 CNRS, IRAP, 9 Av. colonel Roche, BP 44346, F-31028 Toulouse cedex 4, France 6 Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) UMR 5274, Université UJF-Grenoble 1/CNRS-INSU, F-38041 Grenoble, France 7 UMI-FCA, CNRS/INSU, France (UMI 3386), and Dept. de Astronomía, Universidad de Chile, Santiago, Chile e-mail: [email protected] Received September 15, 1996; accepted March 16, 1997 ABSTRACT Aims. Our goal is to determine the molecular composition of the circumstellar disk around AB Aurigae (hereafter, AB Aur). AB Aur is a prototypical Herbig Ae star and the understanding of its disk chemistry is paramount for understanding the chemical evolution of the gas in warm disks. Methods. We used the IRAM 30-m telescope to perform a sensitive search for molecular lines in AB Aur as part of the IRAM Large program ASAI (A Chemical Survey of Sun-like Star-forming Regions). -
Ring Structure in the MWC 480 Disk Revealed by ALMA? Yao Liu1,2, Giovanni Dipierro3, Enrico Ragusa4, Giuseppe Lodato4, Gregory J
A&A 622, A75 (2019) Astronomy https://doi.org/10.1051/0004-6361/201834157 & © ESO 2019 Astrophysics Ring structure in the MWC 480 disk revealed by ALMA? Yao Liu1,2, Giovanni Dipierro3, Enrico Ragusa4, Giuseppe Lodato4, Gregory J. Herczeg5, Feng Long5, Daniel Harsono6, Yann Boehler7,8, Francois Menard8, Doug Johnstone9,10, Ilaria Pascucci11,12, Paola Pinilla13, Colette Salyk14, Gerrit van der Plas8, Sylvie Cabrit8,15, William J. Fischer16, Nathan Hendler11, Carlo F. Manara17, Brunella Nisini18, Elisabetta Rigliaco19, Henning Avenhaus1, Andrea Banzatti11, and Michael Gully-Santiago20 1 Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany 2 Purple Mountain Observatory & Key Laboratory for Radio Astronomy, Chinese Academy of Sciences, 2 West Beijing Road, Nanjing 210008, PR China e-mail: [email protected] 3 Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK 4 Dipartimento di Fisica, Universita` Degli Studi di Milano, Via Celoria, 16, Milano, 20133, Italy 5 Kavli Institute for Astronomy and Astrophysics, Peking University, Yiheyuan 5, Haidian Qu, 100871 Beijing, PR China 6 Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands 7 Rice University, Department of Physics and Astronomy, Main Street, 77005 Houston, USA 8 Université Grenoble Alpes, CNRS, IPAG, 38000 Grenoble, France 9 NRC Herzberg Astronomy and Astrophysics, 5071 West Saanich Road, Victoria, BC, V9E 2E7, Canada 10 Department of Physics and Astronomy, University of Victoria, Victoria, BC, V8P 5C2, Canada -
Nysba Spring 2005 | Vol
NYSBA SPRING 2005 | VOL. 10 | NO. 1 New York International Chapter News A publication of the International Law and Practice Section of the New York State Bar Association A Word From Our A Word From Our Immediate Past Chair New Chair It has been my privilege to Honored and Impressed. have served as Chair of the The first is what I am to be International Law and Practice selected Chair of one of the Section for the past year. I best and most active sections in believe that it has been a pro- the New York State Bar Associ- ductive one in most respects. I ation. The second is what the am especially pleased by the lawyers in New York State and success of the Fall Meeting in around the world are by the Santiago described and pic- members of our Section and its tured elsewhere, our Canadian activities. initiative (including the Execu- Coming off a spectacular tive Committee Retreat in Mon- November 2004 meeting in Santiago de Chile, where we treal, the IL&PS panel at the Barreau de Quebec annual exchanged ideas and mingled with lawyers from almost meeting in Quebec City, the ongoing discussions with every South and Central American country, our Section the Law Society of Upper Canada and the recent Cana- followed up with another terrific substantive program dian Program at the recent IL&PS Annual Meeting), at the NYSBA’s and our Section’s Annual Meeting in and the recognition of the Section’s efforts in recent New York City at the end of January. -
GIARPS High-Resolution Observations of T Tauri Stars (Ghost). II
Astronomy & Astrophysics manuscript no. 38534corr c ESO 2020 August 6, 2020 GIARPS High-resolution Observations of T Tauri stars (GHOsT) II. Connecting atomic and molecular winds in protoplanetary disks Gangi, M.1, Nisini, B.1, Antoniucci, S.1, Giannini, T.1, Biazzo, K.1, Alcalá, J. M.2, Frasca, A.3, Munari, U.4, Arkharov, A. A.5, Harutyunyan, A.6, Manara, C.F.7, Rigliaco, E.8, and Vitali, F.1 1 INAF - Osservatorio Astronomico di Roma - Via Frascati 33, 00078 Monte Porzio Catone, Italy e-mail: [email protected] 2 INAF - Osservatorio Astronomico di Capodimonte - Salita Moiariello 16, 80131 Napoli, Italy 3 INAF - Osservatorio Astrofisico di Catania - Via S. Sofia 78, 95123 Catania, Italy 4 INAF–Osservatorio Astronomico di Padova, via dell’Osservatorio 8, 36012 Asiago (VI), Italy 5 Central Astronomical Observatory of Pulkovo, Pulkovskoe shosse 65, 196140 St. Petersburg, Russia 6 Fundación Galileo Galilei - INAF - Telescopio Nazionale Galileo, 38700 Brena˜ Baja, Santa Cruz de Tenerife, Spain 7 European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany 8 INAF–Osservatorio Astronomico di Padova, vicolo dell’ Osservatorio 5, 35122, Padova, Italy Received Month XX, XXXX; accepted Month XX, XXXX ABSTRACT Aims. In the framework of the GIARPS High-resolution Observations of T Tauri stars (GHOsT) project, we aim to characterize the atomic and molecular winds in a sample of classical T Tauri stars (CTTs) of the Taurus-Auriga region. Methods. We analyzed the flux calibrated [O i] 630 nm and H2 2.12 µm lines in a sample of 36 CTTs observed at the Telescopio Nazionale Galileo with the HARPS and GIANO spectrographs. -
Appendix: Spectroscopy of Variable Stars
Appendix: Spectroscopy of Variable Stars As amateur astronomers gain ever-increasing access to professional tools, the science of spectroscopy of variable stars is now within reach of the experienced variable star observer. In this section we shall examine the basic tools used to perform spectroscopy and how to use the data collected in ways that augment our understanding of variable stars. Naturally, this section cannot cover every aspect of this vast subject, and we will concentrate just on the basics of this field so that the observer can come to grips with it. It will be noticed by experienced observers that variable stars often alter their spectral characteristics as they vary in light output. Cepheid variable stars can change from G types to F types during their periods of oscillation, and young variables can change from A to B types or vice versa. Spec troscopy enables observers to monitor these changes if their instrumentation is sensitive enough. However, this is not an easy field of study. It requires patience and dedication and access to resources that most amateurs do not possess. Nevertheless, it is an emerging field, and should the reader wish to get involved with this type of observation know that there are some excellent guides to variable star spectroscopy via the BAA and the AAVSO. Some of the workshops run by Robin Leadbeater of the BAA Variable Star section and others such as Christian Buil are a very good introduction to the field. © Springer Nature Switzerland AG 2018 M. Griffiths, Observer’s Guide to Variable Stars, The Patrick Moore 291 Practical Astronomy Series, https://doi.org/10.1007/978-3-030-00904-5 292 Appendix: Spectroscopy of Variable Stars Spectra, Spectroscopes and Image Acquisition What are spectra, and how are they observed? The spectra we see from stars is the result of the complete output in visible light of the star (in simple terms). -
Tracing Planet-Induced Structures in Circumstellar Disks Using Molecular Lines
Astronomy & Astrophysics manuscript no. ober2015_astro-ph c ESO 2018 November 5, 2018 Tracing planet-induced structures in circumstellar disks using molecular lines F. Ober1, S. Wolf1, A. L. Uribe2; 3 and H. H. Klahr2 1 Institute of Theoretical Physics and Astrophysics, University of Kiel, Leibnizstraße 15, 24118 Kiel, Germany e-mail: [email protected] 2 Max Planck Institute for Astronomy, Königstuhl, 69117 Heidelberg, Germany 3 University of Chicago, The Department of Astronomy and Astrophysik, 5640 S. Ellis Ave, IL 60637 Chicago Received, 17/03/2015 / Accepted, 11/05/2015 ABSTRACT Context. Circumstellar disks are considered to be the birthplace of planets. Specific structures like spiral arms, gaps, and cavities are characteristic indicators of planet-disk interaction. Investigating these structures can provide insights into the growth of protoplanets and the physical properties of the disk. Aims. We investigate the feasibility of using molecular lines to trace planet-induced structures in circumstellar disks. Methods. Based on 3D hydrodynamic simulations of planet-disk interactions obtained with the PLUTO code, we perform self- consistent temperature calculations and produce N-LTE molecular line velocity-channel maps and spectra of these disks using our new N-LTE line radiative transfer code Mol3D. Subsequently, we simulate ALMA observations using the CASA simulator. We consider two nearly face-on inclinations, five disk masses, seven disk radii, and two different typical pre-main-sequence host stars (T Tauri, Herbig Ae) at a distance of 140 pc. We calculate up to 141 individual velocity-channel maps for five molecules/isotopoloques (12C16O, 12C18O, HCO+, HCN, and CS) in a total of 32 rotational transitions to investigate the frequency dependence of the structures indicated above. -
12899 (Stsci Edit Number: 0, Created: Monday, July 9, 2012 8:35:02 PM EST) - Overview
Proposal 12899 (STScI Edit Number: 0, Created: Monday, July 9, 2012 8:35:02 PM EST) - Overview 12899 - Emission line imaging of the bipolar shell in the Helium Nova V445 Puppis Cycle: 20, Proposal Category: GO (Availability Mode: SUPPORTED) INVESTIGATORS Name Institution E-Mail Dr. Danny Steeghs (PI) (ESA Member) (Contact) The University of Warwick [email protected] Dr. Patrick Woudt (CoI) University of Cape Town [email protected] Dr. Matthew Schurch (CoI) University of Cape Town [email protected] Dr. Margarita Karovska (CoI) (AdminUSPI) Smithsonian Institution Astrophysical Observatory [email protected] Dr. Sumner G. Starrfield (CoI) Arizona State University [email protected] Prof. Thomas R. Marsh (CoI) (ESA Member) The University of Warwick [email protected] Prof. Brian Warner (CoI) University of Cape Town [email protected] Prof. Paul Groot (CoI) (ESA Member) Radboud Universiteit Nijmegen [email protected] VISITS Visit Targets used in Visit Configurations used in Visit Orbits Used Last Orbit Planner Run OP Current with Visit? 01 (1) V-V445-PUP WFC3/UVIS 2 09-Jul-2012 21:34:54.0 yes 2 Total Orbits Used ABSTRACT Explosive detonations on the surfaces of accreting white dwarfs play a key role in establishing viable progenitor pathways towards Type Ia supernova explosions. If the white dwarf is accreting hydrogen deficient material, helium shell-flash driven eruptions can occur on its surface. Thus far only one such helium nova event has been observed in Nova Puppis 2000 = V445 Pup. We have discovered an expanding bipolar shell involving fast moving ejecta of He-rich material surrounding this binary.