DOCSLIB.ORG

Appendix B WIYN 3.5-Meter Publications

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text

Load more

Appendix B WIYN 3.5-meter Publications Papers in Refereed Journals (IU faculty and student authors in bold) Alcalá, J. M., Wachter, S., Covino, E., Sterzik, M. F., Durisen, R. H., Freyberg, M. J., Hoard, D. W., & Cooksey, K., “Multi-Wavelength Observations of the Star Forming Region in L1616,” 2004, A&A, 416, 677. Aoki, W., Frebel, A., Christlieb, N., et al., “HE 1327-2326, an Unevolved Star with [Fe/H]<-5.0. I. A Comprehensive Abundance Analysis,” 2006, ApJ, 639, 897. Austin, S.J., Robertson, J.W., Tycner, C., Campbell, T., & Honeycutt, R.K., "Late-Type Near- Contact Eclipsing Binary [HH97] FS Aur-79", 2007, AJ, 133, 1934 Barrado y Navascues, D., Deliyannis, C. P., & Stauffer, J. R. “WIYN Open Cluster Study 5. Lithium Depletion in K Dwarfs of the M35 Open Cluster,” 2001, ApJ, 549, 452. Barton, E. J., van Zee, L., & Bershady, M. A. 2006, "A Search for Low Surface Brightness Structure around Compact Narrow Emission Line Galaxies," ApJ, 649, 129. Berrington, R. C., Lugger, P. M., & Cohn, H. N. “The Dynamics of the Merging Galaxy Cluster System A2256: Evidence for a New Subcluster,” 2002, AJ, 123, 2261. Deliyannis, C. P., Steinhauer, A., Jeffries, R. D., “Discovery of the Most Lithium-Rich Dwarf: Diffusion in Action,” 2002, ApJ, 577, L39. Dones, L., Showalter, M. R., Durisen, R. H., Honeycutt, R. K., Jurcevic, J. S., Tripoli, R., & Strom, C., “A Search for Saturnian Moonlets Using the WIYN Telescope,” 2005, Icarus, submitted. Drukier, G. A., Slavin, S. D., Cohn, H. N., Lugger, P. M., Berrington, R. C., Murphy, B. W., & Seitzer, P. O., “The Global Kinematics of the Globular Cluster M15,” 1998, AJ, 115, 708. Drukier, G. A., Cohn, H. N., Lugger, P. M., Slavin, S. D., Berrington, R. C., & Murphy, B. W., "The Global Kinematics of the Globular Cluster M92," 2007, AJ, 133, 1041. Guenther, E. W., Stelzer, B., Neuhauser, R., Hillwig, T. C., Durisen, R. H., Menten, K. M., Greimel, R., Barwig, H., Englhauser, J., & Robb, R. M., “A Multi-Wavelength Study of Pre-Main Sequence Stars in the Taurus-Auriga Star-Forming Region,” 2000, A&A, 357, 206. Grindlay, J., Zhao, P., Hong, J., Jenkins, J., Kim, D.-W., Schlegel, E., Drake, J., Kashyap, V., Edmonds, P., Cohn, H., Lugger, P., & Cool, A., “Chandra Multi-wavelength Plane (ChaMPlane) Survey: Design and Initial Results,” Astronomische Nachrichten, 2003, 324, 57. Grindlay, J. E., Hong, J., Zhao, P., Laycock, S., van den Berg, M., Koenig, X., Schlegel, E. M., Cohn, H. N., Lugger, P. M., & Rogel, A. B., “Chandra Multiwavelength Plane (ChaMPlane) Survey: An Introduction,” 2005, ApJ, 635, 920. Harris, W. E., Durrell, P. R., Pierce, M. J., & Secker, J. “The Hubble Constant from Observations of the Brightest Red Giant Stars in a Virgo Cluster Galaxy,” 1998, Nature, 395, 45. Harris, W. M., Combi, M., Honeycutt, R. K., Mueller, B., & Scherb, F., “Evidence for Interacting Gas Flows and an Extended Volatile Source Distribution in the Coma of Comet C/1996 B2 (Hyakutake),” 1997, Science, 277, 676. Hillwig, T. C., Honeycutt, R. K., & Robertson, J. W., “Post Common Envelope Binary Stars and the Pre-Cataclysmic Binary PG 1114+1878,” 2000, AJ, 120, 1113. Hillwig, T. C., Gale, A. A., Honeycutt, R. K. & Rengstorf, A. W., “The Classification and Orbital Period of WD 2154+408: A New Short-Period Post-Common-Envelope Binary,” 2002, PASP, 114, 756. Hillwig, T., Livio, M., & Honeycutt, R. K., “A Search for Collimated Jets in Cataclysmic Variables,” 2004, PASP, 116, 397. Hillwig, T., Robertson, J. W., & Honeycutt, R. K., “Spectroscopic and Photometric Analysis of the Nova-like Cataclysmic Variable PG 1000+667: A New VY Scl. Star,” 1998, AJ, 115, 2044. Hoard, D. W., Szkody, P., Honeycutt, R. K., Robertson, J., Desai, V. & Hillwig, T. “Long-Term Optical and X-Ray Observations of the Old Novae DI Lacertae and V841 Ophiuchi,” 2000, PASP, 112, 1595. Honeycutt, R. K. & Robertson, J. W., “Multiyear Photometry and a Spectroscopic Orbital Period Search for the VY Scl-type Cataclysmic Variable V794 Aquilae,” 1998, AJ, 116, 1961. Honeycutt, R. K., Robertson, J. W., & Turner, G.W., “Unusual 'Stunted' Outbursts in Old Novae and Nova-like Cataclysmic Variables,” 1998, AJ, 115, 2527. Honeycutt, R. K., Robertson, J. W., Turner, G. W., & Henden, A. A., “V446 Herculis (Nova Her 1960) is an Optical Triple: Implications for the Resumption of Dwarf Nova Outbursts Following the Nova,” 1998, ApJ, 495, 933. Jacobson, H. R., C. A. Pilachowski, and E. D. Friel, "Na, Al, and O abundances of Open Clusters NGC 7142, NGC 6939, and IC 4756," 2007, AJ (in press). Jurcevic, J. S., Pierce, M. J., & Jacoby, G. H., “Distances via Red Supergiant Variables. II. M101,” 2000, MNRAS, 313, 868. Johnson, C.I., Kraft, R.P., Pilachowski, C. A., Sneden, C., Ivans, I.I., Benman, G., “A 235 Star Sample Sodium, Magnesium, and Aluminum Abundance Study in the Globular Clusters M3 (NGC 5272) and M13 (NGC 6205),” 2005, PASP 117, 1308-1324. Johnson, C. I.; Pilachowski, C. A. 2006, "A Moderate Sample Size, Multielement Analysis of the Globular Cluster M12 (NGC 6218)," 2006, AJ, 132, 2346. Kafka, S., Tappert, C., Honeycutt, R. K., & Bianchini, A., “Spectroscopic Study of Q Cygni: Surprises from an Old Nova,” 2003, AJ, 126, 1472. Kafka, S. & Honeycutt, R. K., “WIYN Open Cluster Study. XV. Photometric Monitoring of Open Clusters: New Variables in NGC 188,” 2003, AJ, 126, 276. Kafka, S. & Honeycutt, R. K., “Stellar Activity in the Lower Main Sequence in Praesepe,” Astronomische Nachrichten, 2004, 325, 413. Kafka, S. & Honeycutt, R.K. "Detecting Outflows from Cataclysmic Variables in the Optical", 2004, AJ, 128, 2420. Kafka, S., Robertson, J., Honeycutt, R. K., & Howell, S. B., “Low-State Flaring Events in AM Her,” 2005, AJ, 129, 2411. Kafka, S., Honeycutt, R. K., Howell, S. B., Harrison, T. E., “A Multiwavelength Study of AM Herculis during the 2002-2004 Low States,” 2005, AJ, 130, 2852-2865. Kafka, S., Honeycutt, R.K., Howell, S.B., “Continued Hyperactivity on the Secondary Star of AM Herculis,” 2006, AJ, 131, 2673. Kafka, S., & Honeycutt, R.K., "Spectroscopy of Active and Inactive M Dwarfs in Praesepe", 2006, AJ, 132, 1517. Kafka, S., Honeycutt, R.K, & Howell, S.B., "Continued Hyperactivity on the Secondary Star of AM Herculis", 2006, AJ, 131, 2673. Kafka, S., Howell, S.B., Honeycutt, R.K., & Robertson, J.W. "A Photometric and Spectroscopic Study of the Cataclysmic Variable ST LMi during 2005-2006", 2007, AJ, 133, 1645. Lugger, P. M., Cohn, H. N., Heinke, C. O., Grindlay, J. E., & Edmonds, P. D., "Chandra X-ray Sources in the Collapsed-Core Globular Cluster M30 (NGC 7099)," 2007, ApJ, 657, 286. McArthur, B., Benedict, G. F., Lee, J., Lu, C., van Altena, W. F., Deliyannis, C. P., Girard, T., Fredrick, L. W., Nelan, E., Duncombe, R. L., Hemenway, P. D., Jefferys, W. H., Shelus, P. S., Franz, O. G., & Wasserman, L., 1999, “Astrometry with Hubble Space Telescope Fine Guidance Sensor 3: The Parallax of the Cataclysmic Variable RW Triangulum,” ApJ, 520, L59. Nair, P. H., Kafka, S., Honeycutt, R. K., & Gilliland, R. L., “Cataclysmic Variables in Open Clusters: EU Cnc,” 2005 International Bulletin On Variable Stars, 5585, 1. Pierce, M. J. & Berrington, R. C., “Evidence for Stellar Streaming in the Cores of Elliptical Galaxies: A Relic Kinematic Signature of Mergers,” 2000, ApJ, 531, L99. Pierce, M. J., Jurcevic, J. S., & Crabtree, D., “Distances via Red Supergiant Variables. I. A Period Luminosity Relation at Optical Wavelengths,” 2000, MNRAS, 313, 271. Platais, I., Kozhurina-Platais, V., Girard, T. M., Demarque, P., van Altena, W. F., Barnes, S., Deliyannis, C. P., & Horch, E., “WIYN Open Cluster Study 7. NGC 2451A and the Hipparcos Distance Scale,” 2001, AJ, 122, 1486. Rengstorf, A.W., “Quasar Detection via Variability in a High Galactic Latitude Drift Scan Survey,” 2004, PASP, 116, 103. Rengstorf, A. W., Mufson, S. L., Abad, C., Adams, B., Andrews, P., Bailyn, C., Baltay, C., Bongiovanni, A., Briceño, C., Bruzual, G., Coppi, P., della Prugna, F., Emmet, W., Ferrín, I., Fuenmayor, F., Gebhard, M., Hernández, J., Honeycutt, R. K., Magris, G., Musser, J., Naranjo, O., Oemler, A., Rosenzweig, P., Sabbey, C. N., Sánchez, Ge., Sánchez, Gu., Schaefer, B., Schenner, H., Sinnott, J., Snyder, J. A., Sofia, S., Stock, J., van Altena, W., Vivas, A. K., “New Quasars Detected via Variability in the QUEST1 Survey,” 2004, ApJ, 606, 741. Rengstorf, A.W. et al., “QUEST1 Variability Survey. II. Variability Determination Criteria and 200k Light Curve Catalog,” 2004, ApJ, 617, 184. Robertson, J. W., Honeycutt, R. K., Hillwig, T., Jurcevic, J. S., & Henden, A. H. “Reconnaissance of Suspected Old Novae,” 2000, AJ, 119, 1365. Rogel, A. B., Lugger, P. M., Cohn, H. N., Slavin, S. D., Grindlay, J. E., Zhao, P., & Hong, J., “Three Years of ChaMPlane Northern Field WIYN Spectroscopy,” 2006, ApJ, 163, 160. Sabbey, C. N., Oemler, A., Coppi, P., Baltay, C., Bongiovanni, A., Bruzual, G., Garcia, C. E., Musser, J., Rengstorf, A. W., & Snyder, J. A., “The Low-Redshift Quasar-Quasar Correlation Function from an Extragalactic Hα Emission-Line Survey to z=0.4,” 2001, ApJ, 548, 585. Schaefer, B. E., King, J. R., & Deliyannis, C. P., “Superflares on Ordinary Solar-Type Stars,” 2000, ApJ, 529, 1026. Schaefer, B. E. et al., “The Discovery of the Optical Transient of the Gamma Ray Burst 990308,” 1999, ApJ, 524, L103. Shara, M. M., Martin, C. D., Seibert, M., Rich, M., Salim, S., Reitzel, D., Schiminovich, D., Deliyannis, C. P., Sarrazine, A. R., Kulkarni, S. R., Ofek, E. O., Brosch, N., Lépine, S., Zurek, D., De Marco, O., Jacoby, G. 2007, “An Ancient Nova Shell Surrounds the Prototypical Dwarf Nova Z Cam," Nature, 446, 159. Sills, A. & Deliyannis, C. P. “WIYN Open Cluster Study 6.
Recommended publications
  • A Basic Requirement for Studying the Heavens Is Determining Where In

    A Basic Requirement for Studying the Heavens Is Determining Where In

    Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun­ damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short).
  • Übersicht NGC-Objektauswahl Cepheus Zur Übersichtskarte

    Übersicht NGC-Objektauswahl Cepheus Zur Übersichtskarte

    NGC-Objektauswahl Cepheus NGC 40 NGC 7055 NGC 7354 NGC 188 NGC 7076 NGC 7380 NGC 1184 NGC 7129 NGC 7419 NGC 1544 NGC 7139 NGC 7423 NGC 2276 NGC 7142 NGC 7429 NGC 2300 NGC 7160 NGC 7510 NGC 6939 NGC 7226 NGC 7538 NGC 6949 NGC 7235 NGC 7708 NGC 6951 NGC 7261 NGC 7762 NGC 7023 NGC 7281 NGC 7822 Sternbild- Übersicht Zur Objektauswahl: Nummer anklicken Zur Übersichtskarte: Objekt anklicken Sternbildübersicht Auswahl NGC 40_7708 Aufsuchkarte Auswahl NGC 188_Aufsuchkarte 2 UMi 2 Auswahl NGC 1184 Aufsuchkarte Auswahl NGC 1544_2276_2300 Aufsuchkarte Auswahl NGC 6939 Aufsuchkarte Auswahl NGC 6949_6951 Aufsuchkarte Auswahl NGC 7023 Aufsuchkarte Auswahl NGC 7055 Aufsuchkarte Auswahl NGC 7076 Aufsuchkarte Auswahl NGC 7129_7142 Aufsuchkarte Auswahl NGC 7139_7160 Aufsuchkarte Auswahl NGC 7226_7235 Aufsuchkarte Auswahl N 7261_7281 Aufsuchkarte Auswahl NGC 7354_7419_7429_7510_7538 Aufsuchkarte Auswahl NGC 7380_7423 Aufsuchkarte Auswahl NGC 7762_7822 Aufsuchkarte Auswahl NGC 40 Übersichtskarte Aufsuch- Auswahl karte NGC 188 Übersichtskarte Aufsuch- Auswahl karte NGC 1184 Übersichtskarte Aufsuch- Auswahl karte NGC 1544 Übersichtskarte Aufsuch- Auswahl karte N 2276_N 2300 Übersichtskarte Aufsuch- Auswahl karte NGC 6939 Übersichtskarte Aufsuch- Auswahl karte NGC 6949 Übersichtskarte Aufsuch- Auswahl karte NGC 6951 Übersichtskarte Aufsuch- Auswahl karte NGC 7023 Übersichtskarte Aufsuch- Auswahl karte NGC 7055 Übersichtskarte Aufsuch- Auswahl karte NGC 7076 Übersichtskarte Aufsuch- Auswahl karte NGC 7129_7142 Übersichtskarte Aufsuch- Auswahl karte NGC 7139
  • Newsletter Archive the Skyscraper October 2018

    Newsletter Archive the Skyscraper October 2018

    the vol. 45 no. 10 Skyscraper October 2018 AMATEUR ASTRONOMICAL SOCIETY OF RHODE ISLAND 47 PEEPTOAD ROAD NORTH SCITUATE, RHODE ISLAND 02857 WWW.THESKYSCRAPERS.ORG In This Issue: 2 Upcoming Meetings 2 Skyscrapers Library Update 3 Moon Maps 4 Observe the Moon 5 The Sun, Moon & Planets in October 6 October Meteor Showers & Still Time to Observe Mars and Saturn 7 On the Change of Seasons 8 NGC 7129 : Cluster & Nebula in Cepheus Saturday, October 20, 7:00pm 9 August Reports at Seagrave Observatory 9 My First Telescope: A Every year, astronomers dedicate one night to really concentrate on our Family Program only natural satellite, the Moon. Observatories around the world will be enjoying the sight of the Moon, in its waxing gibbous phase. Seagrave Memorial Observatory will have its beautiful 1878 8-inch Clark refractor and other telescopes open for the evening. Members of Skyscrap- ers, Inc., guardians of Seagrave Memorial Observatory, will be available to interpret your observations, to make your visit truly a night to remember. Come and be a part of a worldwide effort to introduce, and appreciate, our Phases of the Moon nearest celestial neighbor. Last Quarter Moon October 2 09:45 New Moon October 9 03:47 Seagrave Memorial First Quarter Moon Observatory October 16 18:02 Open Nights Full Hunter's Moon October 24 16:45 Saturdays st 7:00 pm Last Quarter Moon weather permitting October 31 16:40 Upcoming Meetings Skyscrapers Library Update Friday, November 2: Seagrave Observatory Thanks to member Roger Forsythe for his donation of books to Diana Hannikainen: "Stepping Through the Cosmos" our library a couple of months ago.
  • International Astronomical Union Commission G1 BIBLIOGRAPHY of CLOSE BINARIES No

    International Astronomical Union Commission G1 BIBLIOGRAPHY of CLOSE BINARIES No

    International Astronomical Union Commission G1 BIBLIOGRAPHY OF CLOSE BINARIES No. 104 Editor-in-Chief: W. Van Hamme Editors: R.H. Barb´a D.R. Faulkner P.G. Niarchos D. Nogami R.G. Samec C.D. Scarfe C.A. Tout M. Wolf M. Zejda Material published by March 15, 2017 BCB issues are available at the following URLs: http://ad.usno.navy.mil/wds/bsl/G1_bcb_page.html, http://faculty.fiu.edu/~vanhamme/IAU-BCB/. The bibliographical entries for Individual Stars and Collections of Data, as well as a few General entries, are categorized according to the following coding scheme. Data from archives or databases, or previously published, are identified with an asterisk. The observation codes in the first four groups may be followed by one of the following wavelength codes. g. γ-ray. i. infrared. m. microwave. o. optical r. radio u. ultraviolet x. x-ray 1. Photometric data a. CCD b. Photoelectric c. Photographic d. Visual 2. Spectroscopic data a. Radial velocities b. Spectral classification c. Line identification d. Spectrophotometry 3. Polarimetry a. Broad-band b. Spectropolarimetry 4. Astrometry a. Positions and proper motions b. Relative positions only c. Interferometry 5. Derived results a. Times of minima b. New or improved ephemeris, period variations c. Parameters derivable from light curves d. Elements derivable from velocity curves e. Absolute dimensions, masses f. Apsidal motion and structure constants g. Physical properties of stellar atmospheres h. Chemical abundances i. Accretion disks and accretion phenomena j. Mass loss and mass exchange k. Rotational velocities 6. Catalogues, discoveries, charts a. Catalogues b. Discoveries of new binaries and novae c.
  • Wide-Field Plate Archive of the University Observatory Jena

    Wide-Field Plate Archive of the University Observatory Jena

    Astron. Nachr. / AN 999, No.88, 789–794 (2014) / DOI please set DOI! Wide-Field Plate Archive of the University Observatory Jena ⋆ A.V. Poghosyan1, W. Pfau1, K.P. Tsvetkova2, M. Mugrauer1, M.K. Tsvetkov2,3, V.V. Hambaryan1,⋆⋆, R. Neuhauser¨ 1, and D.G.Kalaglarsky2 1 Astrophysikalisches Institut und Universit¨ats-Sternwarte Jena, Schillerg¨aß chen 2, D-07745 Jena, Germany 2 Institute of Mathematics and Informatics, Bulgarian Academy of Sciences, Sofia 1113, Bulgaria 3 Institute of Astronomy, Bulgarian Academy of Sciences, Sofia 1784, Bulgaria Received 17 Feb 2014, accepted 19 Mar 2014 Published online later Key words astronomical databases: catalogs We present the archive of the wide-field plate observations obtained at the University Observatory Jena, which is stored at the Astrophysical Institute of the Friedrich Schiller University Jena. The archive contains plates taken in the period February 1963 to December 1982 with the 60/90/180-cm Schmidt telescope of the university observatory. A computer- readable version of the plate metadata catalogue (for 1257 plates), the logbooks, as well as the digitized Schmidt plates in low and high resolution are now accessible to the astronomical community.This paper describes the properties of the archive, as well as the processing procedure of all plates in detail. c 2014 WILEY-VCH Verlag GmbH& Co. KGaA, Weinheim 1 Introduction Großschwabhausen,about 10 km to the west of Jena. Archi- tect of the telescope building was Hans Schlag, an architect The large astronomical plate collections provide unique re- who together with J. Schreiter is also famous for the Plan- sources for photometric and astrometric studies of astro- etarium in Jena, built in 1926.
  • Prof.Dr. Ahmet Talat SAYGAÇ

    Prof.Dr. Ahmet Talat SAYGAÇ

    Prof.Dr. Ahmet Talat SAYGAÇ Kişisel Bilgiler Fİşa xT eTlelfeofnoun:u +: 9+09 201 221 424 404 00 00307 D0 ahili: 10282 WE-epbo:s that:t pssa:/y/[email protected]/astronomy PVoezsntaec Ailedrr -e Fsia:t iİhs t-a İnsbtaunl bÜunliversitesi (Rektörlük Bahçe İçi), Fen Fakültesi, Astronomi ve Uzay Bilimleri Bölümü, 34134 - Beyazıt - Eğitim Bilgileri YDüokksteokr aL, iİssatnans,b İustl aÜnnbiuvel rÜsnitievseir, sFiteens iB, Filiemnl eBrilii mEnlesrtiit üEsnüs,t iAtüsstrüo, nAosmtroi Vnoe mUiz aVye BUizliamyl eBrilii mBölelürim, Tüü, rTküirykei y1e9 8119 8- 31 9- 813994 ÖLins aLnisa, nEsg,e E Üdnirinver Esğitietismi, FEenns tFitaüksüül,t eFsizi,i kA s- tKroimnyoam -i BViey oUlzoajiy, TBüilrimkilyeer i1 B9ö7l4ü m- 1ü9, 7T5ürkiye 1975 - 1980 Yİnagbiliazcnec, Bı 2D Oilrltea rÜstü Yaptığı Tezler EDnoskttiotürsaü, ,V AWst rHoyndormi Ki aVtea kUlizsamy iBk iDlimeğleişrei,n 1 Y9ı9ld4ızın Optik ve Morötesi Tayfsal Analizi, İstanbul Üniversitesi, Fen Bilimleri BYüilikmselekr Li, i1sa9n8s3, SA 57 Alanının RGU Fotometrisi, İstanbul Üniversitesi, Fen Bilimleri Enstitüsü, Astronomi Ve Uzay ABirliamş, tTıerkmnoalo Aji lvaen Tloaprlıum, Eğitim, Fizik, Astronomi ve Astrofizik, Güneş ve Güneş Sistemleri, Temel Astronomi ve dAısştır noefisznike:l eErn vster üsimstaenmtalesry;oevnr, eTne,k Ynıilkdlıezrla vre, TAesmtreoln Boimlimikl egrözlemler, Yıldız Sistemleri;Yıldızlararası ortam;galaktik ve galaksi Akademik Unvanlar / Görevler DProoçf.D.Drr.,. , İİssttaannbbuull ÜÜnniivveerrssiitteessii, , FFeenn FFaakküülltteessii, , AAssttrroonnoommii
  • Titles Promote Sustainable Initiatives

    Titles Promote Sustainable Initiatives

    Student Research Poster Symposium April 8, 2011 Villanova University Sigma Xi Research Poster Symposium, April 8, 2011 2 Proceedings of the 2011 Student Research Symposium April 8, 2011 Villanova Room Villanova University Villanova, PA 19085 USA Supported by: The Villanova Chapter of Sigma Xi, the Scientific Research Society Sigma Xi Research Poster Symposium, April 8, 2011 This volume is also available electronically on the Sigma Xi chapter’s website, http://www.csc.villanova.edu/~sigmaxi/ Sigma Xi Research Poster Symposium, April 8, 2011 4 Welcome from the Poster Symposium Organizers Welcome to the 2010 Villanova University Sigma Xi’s Student Research Poster Symposium! Sigma Xi is the international honor society for research scientists and engineers. The Villanova chapter of Sigma Xi is proud to sponsor this poster symposium event to recognize and celebrate the research work accomplished by our students, and to give students an opportunity to further develop their skills in communicating those accomplishments. This book contains abstracts of 56 contributed posters. Outstanding posters will be recognized in the form of poster awards. Many thanks to all students who contributed to this symposium. We gratefully acknowledge the dedicated poster judges who committed to evaluating the research posters and providing written feedback at the end of the symposium. Special thanks for their time and commitment to promoting research at Villanova University! Congratulations to all! Mirela Damian Sigma Xi Chapter President Anil Bamezai Sigma Xi Chapter President-Elect Sridhar Santhanam Sigma Xi Chapter Secretary-Treasurer Sigma Xi Research Poster Symposium, April 8, 2011 Table of Contents Astronomy and Astrophysics (5) Ultraviolet Spectral Synthesis of HgMn Stars.
  • SAC's 110 Best of the NGC

    SAC's 110 Best of the NGC

    SAC's 110 Best of the NGC by Paul Dickson Version: 1.4 | March 26, 1997 Copyright °c 1996, by Paul Dickson. All rights reserved If you purchased this book from Paul Dickson directly, please ignore this form. I already have most of this information. Why Should You Register This Book? Please register your copy of this book. I have done two book, SAC's 110 Best of the NGC and the Messier Logbook. In the works for late 1997 is a four volume set for the Herschel 400. q I am a beginner and I bought this book to get start with deep-sky observing. q I am an intermediate observer. I bought this book to observe these objects again. q I am an advance observer. I bought this book to add to my collect and/or re-observe these objects again. The book I'm registering is: q SAC's 110 Best of the NGC q Messier Logbook q I would like to purchase a copy of Herschel 400 book when it becomes available. Club Name: __________________________________________ Your Name: __________________________________________ Address: ____________________________________________ City: __________________ State: ____ Zip Code: _________ Mail this to: or E-mail it to: Paul Dickson 7714 N 36th Ave [email protected] Phoenix, AZ 85051-6401 After Observing the Messier Catalog, Try this Observing List: SAC's 110 Best of the NGC [email protected] http://www.seds.org/pub/info/newsletters/sacnews/html/sac.110.best.ngc.html SAC's 110 Best of the NGC is an observing list of some of the best objects after those in the Messier Catalog.
  • Open Clusters

    Open Clusters

    Open Clusters Open clusters (also known as galactic clusters) are of tremendous importance to the science of astronomy, if not to astrophysics and cosmology generally. Star clusters serve as the "laboratories" of astronomy, with stars now all at nearly the same distance and all created at essentially the same time. Each cluster thus is a running experiment, where we can observe the effects of composition, age, and environment. We are hobbled by seeing only a snapshot in time of each cluster, but taken collectively we can understand their evolution, and that of their included stars. These clusters are also important tracers of the Milky Way and other parent galaxies. They help us to understand their current structure and derive theories of the creation and evolution of galaxies. Just as importantly, starting from just the Hyades and the Pleiades, and then going to more distance clusters, open clusters serve to define the distance scale of the Milky Way, and from there all other galaxies and the entire universe. However, there is far more to the study of star clusters than that. Anyone who has looked at a cluster through a telescope or binoculars has realized that these are objects of immense beauty and symmetry. Whether a cluster like the Pleiades seen with delicate beauty with the unaided eye or in a small telescope or binoculars, or a cluster like NGC 7789 whose thousands of stars are seen with overpowering wonder in a large telescope, open clusters can only bring awe and amazement to the viewer. These sights are available to all.
  • International Astronomical Union Commission G1 BIBLIOGRAPHY

    International Astronomical Union Commission G1 BIBLIOGRAPHY

    International Astronomical Union Commission G1 BIBLIOGRAPHY OF CLOSE BINARIES No. 108 Editor-in-Chief: W. Van Hamme Editors: R.H. Barb´a D.R. Faulkner P.G. Niarchos D. Nogami R.G. Samec C.D. Scarfe C.A. Tout M. Wolf M. Zejda Material published by March 15, 2019 BCB issues are available at the following URLs: http://ad.usno.navy.mil/wds/bsl/G1_bcb_page.html, http://faculty.fiu.edu/~vanhamme/IAU-BCB/. The bibliographical entries for Individual Stars and Collections of Data, as well as a few General entries, are categorized according to the following coding scheme. Data from archives or databases, or previously published, are identified with an asterisk. The observation codes in the first four groups may be followed by one of the following wavelength codes. g. γ-ray. i. infrared. m. microwave. o. optical r. radio u. ultraviolet x. x-ray 1. Photometric data a. CCD b. Photoelectric c. Photographic d. Visual 2. Spectroscopic data a. Radial velocities b. Spectral classification c. Line identification d. Spectrophotometry 3. Polarimetry a. Broad-band b. Spectropolarimetry 4. Astrometry a. Positions and proper motions b. Relative positions only c. Interferometry 5. Derived results a. Times of minima b. New or improved ephemeris, period variations c. Parameters derivable from light curves d. Elements derivable from velocity curves e. Absolute dimensions, masses f. Apsidal motion and structure constants g. Physical properties of stellar atmospheres h. Chemical abundances i. Accretion disks and accretion phenomena j. Mass loss and mass exchange k. Rotational velocities 6. Catalogues, discoveries, charts a. Catalogues b. Discoveries of new binaries and novae c.
  • Publications of Variable Star Section, Royal

    Publications of Variable Star Section, Royal

    J No. 11 (C83)J 4 5 o i o 3 a —i—|—r FIGURE 5 PUBLICATIONS of 7 VARIABLE STAR SEQTI ROYAL ASTRONOMICAL SOCIETY OF NEW ZEALAND 10 to u 11 1% '3 1 liiii o o 0 0 34 NO Nj> • • C -t- T T m to GU JU Mm SGR it Director: Frank M. Bateson P.O. Box 3093, GREERTON, TAURANGA, ft- NEW ZEALAND. i CONTENTS. PAGE THE LIGHT CURVE OF OY CARINAE, 1963 June 15 to 1983 May 31. Frank M. Bateson & A.W. Dodson 1 VISUAL OBSERVATIONS OF THE ECLIPSES OF THE DWARF NOVA OY CARINAE. N.W. Taylor & A.C. Gilmore 14 U HOROLOGII—A NEGLECTED MIRA VARIABLE. C.W. Venimore 22 PHOTOELECTRIC UBV SEQUENCES FOR FOUR SUSPECTED RCB STARS. David Kilkenny 29 PHOTOELECTRIC PHOTOMETRY OF V856 SCORPII & NEARBY SEQUENCE STARS. Brian F. Marino & W.S.G. Walker 31 VISUAL OBSERVATIONS OF V818 SCORPII (Sco X-l) 1974- 1982. Frank M. Bateson & C.W. Venimore 35 THE SEMI-REGULAR VARIABLE, RX RETICULI. A.W. Dodson 45 COLOURS FOR THE VARIABLE STAR V384 CARINAE. Brian F. Marino & W.S.G. Walker 48 REPORT ON SOME NOVAE & SUSPECTED RECURRENT NOVAE. Frank M. Bateson 51 A VISUAL ATLAS OF THE LARGE MAGELLANIC CLOUD. Mati Morel 62 LIGHT CURVE OF NOVA MUSCAE 1983. Frank M. Bateson & A.W. Dodson 65 ASTRONOMICAL RESEARCH LIMITED Frank M. Bateson 69 REPORT OF THE VARIABLE STAR SECTION, ROYAL ASTRONOMICAL SOCIETY OF NEW ZEALAND FOR YEAR ENDED 1983 December 31 70 PUBLISHED BY ASTRONOMICAL RESEARCH LIMITED P.O. BOX 3093, GREERTON TAURANGA, NEW ZEALAND.
  • (Ap) Mag Size Distance Rise Transit Set Gal NGC 6217 Arp 185 Umi

    (Ap) Mag Size Distance Rise Transit Set Gal NGC 6217 Arp 185 Umi

    Herschel 400 Observing List, evening of 2015 Oct 15 at Cleveland, Ohio Sunset 17:49, Twilight ends 19:18, Twilight begins 05:07, Sunrise 06:36, Moon rise 09:51, Moon set 19:35 Completely dark from 19:35 to 05:07. Waxing Crescent Moon. All times local (EST). Listing All Classes visible above the perfect horizon and in twilight or moonlight before 23:59. Cls Primary ID Alternate ID Con RA (Ap) Dec (Ap) Mag Size Distance Rise Transit Set Gal NGC 6217 Arp 185 UMi 16h31m48.9s +78°10'18" 11.9 2.6'x 2.1' - 15:22 - Gal NGC 2655 Arp 225 Cam 08h57m35.6s +78°09'22" 11 4.5'x 2.8' - 7:46 - Gal NGC 3147 MCG 12-10-25 Dra 10h18m08.0s +73°19'01" 11.3 4.1'x 3.5' - 9:06 - PNe NGC 40 PN G120.0+09.8 Cep 00h13m59.3s +72°36'43" 10.7 1.0' 3700 ly - 23:03 - Gal NGC 2985 MCG 12-10-6 UMa 09h51m42.0s +72°12'01" 11.2 3.8'x 3.1' - 8:39 - Gal Cigar Galaxy M 82 UMa 09h57m06.5s +69°35'59" 9 9.3'x 4.4' 12.0 Mly - 8:45 - Gal NGC 1961 Arp 184 Cam 05h43m51.6s +69°22'44" 11.8 4.1'x 2.9' 180.0 Mly - 4:32 - Gal NGC 2787 MCG 12-9-39 UMa 09h20m40.5s +69°07'51" 11.6 3.2'x 1.8' - 8:09 - Gal NGC 3077 MCG 12-10-17 UMa 10h04m31.3s +68°39'09" 10.6 5.1'x 4.2' 12.0 Mly - 8:52 - Gal NGC 2976 MCG 11-12-25 UMa 09h48m29.2s +67°50'21" 10.8 6.0'x 3.1' 15.0 Mly - 8:36 - PNe Cat's Eye Nebula NGC 6543 Dra 17h58m31.7s +66°38'25" 8.3 22" 4400 ly - 16:49 - Open NGC 7142 Collinder 442 Cep 21h45m34.2s +65°51'16" 10 12.0' 5500 ly - 20:35 - Gal NGC 2403 MCG 11-10-7 Cam 07h38m20.9s +65°33'36" 8.8 20.0'x 10.0' 11.0 Mly - 6:26 - Open NGC 637 Collinder 17 Cas 01h44m15.4s +64°07'07" 7.3 3.0' 7000 ly - 0:33