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NASA's Goddard Space Flight Center Laboratory for High Energy
1 NASA’s Goddard Space Flight Center Laboratory for High Energy Astrophysics Greenbelt, Maryland 20771 @S0002-7537~99!00301-7# This report covers the period from July 1, 1997 to June 30, Toshiaki Takeshima, Jane Turner, Ken Watanabe, Laura 1998. Whitlock, and Tahir Yaqoob. This Laboratory’s scientific research is directed toward The following investigators are University of Maryland experimental and theoretical research in the areas of X-ray, Scientists: Drs. Keith Arnaud, Manuel Bautista, Wan Chen, gamma-ray, and cosmic-ray astrophysics. The range of inter- Fred Finkbeiner, Keith Gendreau, Una Hwang, Michael Loe- ests of the scientists includes the Sun and the solar system, wenstein, Greg Madejski, F. Scott Porter, Ian Richardson, stellar objects, binary systems, neutron stars, black holes, the Caleb Scharf, Michael Stark, and Azita Valinia. interstellar medium, normal and active galaxies, galaxy clus- Visiting scientists from other institutions: Drs. Vadim ters, cosmic-ray particles, and the extragalactic background Arefiev ~IKI!, Hilary Cane ~U. Tasmania!, Peter Gonthier radiation. Scientists and engineers in the Laboratory also ~Hope College!, Thomas Hams ~U. Seigen!, Donald Kniffen serve the scientific community, including project support ~Hampden-Sydney College!, Benzion Kozlovsky ~U. Tel such as acting as project scientists and providing technical Aviv!, Richard Kroeger ~NRL!, Hideyo Kunieda ~Nagoya assistance to various space missions. Also at any one time, U.!, Eugene Loh ~U. Utah!, Masaki Mori ~Miyagi U.!, Rob- there are typically between twelve and eighteen graduate stu- ert Nemiroff ~Mich. Tech. U.!, Hagai Netzer ~U. Tel Aviv!, dents involved in Ph.D. research work in this Laboratory. Yasushi Ogasaka ~JSPS!, Lev Titarchuk ~George Mason U.!, Currently these are graduate students from Catholic U., Stan- Alan Tylka ~NRL!, Robert Warwick ~U. -
Case 20-32299-KLP Doc 208 Filed 06/01/20 Entered 06/01/20 16
Case 20-32299-KLP Doc 208 Filed 06/01/20 Entered 06/01/20 16:57:32 Desc Main Document Page 1 of 137 Case 20-32299-KLP Doc 208 Filed 06/01/20 Entered 06/01/20 16:57:32 Desc Main Document Page 2 of 137 Exhibit A Case 20-32299-KLP Doc 208 Filed 06/01/20 Entered 06/01/20 16:57:32 Desc Main Document Page 3 of 137 Exhibit A1 Served via Overnight Mail Name Attention Address 1 Address 2 City State Zip Country Aastha Broadcasting Network Limited Attn: Legal Unit213 MezzanineFl Morya LandMark1 Off Link Road, Andheri (West) Mumbai 400053 IN Abs Global LTD Attn: Legal O'Hara House 3 Bermudiana Road Hamilton HM08 BM Abs-Cbn Global Limited Attn: Legal Mother Ignacia Quezon City Manila PH Aditya Jain S/O Sudhir Kumar Jain Attn: Legal 12, Printing Press Area behind Punjab Kesari Wazirpur Delhi 110035 IN AdminNacinl TelecomunicacionUruguay Complejo Torre De Telecomuniciones Guatemala 1075. Nivel 22 HojaDeEntrada 1000007292 5000009660 Montevideo CP 11800 UY Advert Bereau Company Limited Attn: Legal East Legon Ars Obojo Road Asafoatse Accra GH Africa Digital Network Limited c/o Nation Media Group Nation Centre 7th Floor Kimathi St PO Box 28753-00100 Nairobi KE Africa Media Group Limited Attn: Legal Jamhuri/Zaramo Streets Dar Es Salaam TZ Africa Mobile Network Communication Attn: Legal 2 Jide Close, Idimu Council Alimosho Lagos NG Africa Mobile Networks Cameroon Attn: Legal 131Rue1221 Entree Des Hydrocarbures Derriere Star Land Hotel Bonapriso-Douala Douala CM Africa Mobile Networks Cameroon Attn: Legal BP12153 Bonapriso Douala CM Africa Mobile Networks Gb, -
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Baltic Astronomy, vol. 19, 95{110, 2010 CHEMICAL COMPOSITION OF THE RS CVn-TYPE STAR LAMBDA ANDROMEDAE G. Tautvaiˇsien_e1, G. Bariseviˇcius1, S. Berdyugina2, Y. Chorniy1 and I. Ilyin3 1 Institute of Theoretical Physics and Astronomy, Vilnius University, Goˇstauto12, Vilnius LT-01108, Lithuania 2 Kiepenheuer Institut f¨urSonnenphysik, Sch¨oneckstrasse 6, Freiburg D-79104, Germany 3 Astrophysical Institute Potsdam, An der Sternwarte 16, Potsdam D-14482, Germany Received: 2010 June 8; accepted: 2010 June 15 Abstract. Photospheric parameters and chemical composition are deter- mined for the single-lined chromospherically active RS CVn-type star λ And (HD 222107). From the high resolution spectra obtained on the Nordic Optical Telescope, abundances of 22 chemical elements and isotopes, including such key elements as 12C, 13C, N and O, were investigated. The differential line analysis with the MARCS model atmospheres gives Teff = 4830 K, log g = 2.8, [Fe/H] = {0.53, [C/Fe] = 0.09, [N/Fe] = 0.35, [O/Fe] = 0.45, C/N = 2.21, 12C/13C = 14. The 12C/13C ratio for a star of the RS CVn-type is determined for the first time, and its low value gives a hint that extra-mixing processes may start acting in low-mass chromospherically active stars below the bump of the luminosity function of red giants. Key words: stars: RS CVn binaries, abundances { stars: individual (λ And = HD 222107) 1. INTRODUCTION The RS CVn-type stars have been studied thoroughly since 1965 when their peculiar light curves were detected (Rodon´o1965; Chisari & Lacona 1965) and a new distinct class of binaries was named (Olivier 1974; Hall 1976). -
Jahresbericht 2010 Mitteilungen Der Astronomischen Gesellschaft 94 (2013), 583–627
Jahresbericht 2010 Mitteilungen der Astronomischen Gesellschaft 94 (2013), 583–627 Potsdam Leibniz-Institut für Astrophysik Potsdam (AIP) An der Sternwarte 16, D-14482 Potsdam Tel. 03317499-0, Telefax: 03317499-267 E-Mail: [email protected] WWW: http://www.aip.de Beobachtungseinrichtungen Robotisches Observatorium STELLA Observatorio del Teide, Izaña E-38205 La Laguna, Teneriffa, Spanien Tel. +34 922 329 138 bzw. 03317499-633 LOFAR-Station DE604 Potsdam-Bornim D-14469 Potsdam Tel. 03317499-291, Telefax: 03317499-352 Observatorium für Solare Radioastronomie Tremsdorf D-14552 Tremsdorf Tel. 03317499-291, Telefax: 03317499-352 Sonnenobservatorium Einsteinturm Telegrafenberg, D-14473 Potsdam Tel. 0331288-2303/-2304, Telefax: 03317499-524 0 Allgemeines Das Leibniz-Institut für Astrophysik Potsdam (AIP) ist eine Stiftung bürgerlichen Rechts zum Zweck der wissenschaftlichen Forschung auf dem Gebiet der Astrophysik. Als außer- universitäre Forschungseinrichtung ist es Mitglied der Leibniz-Gemeinschaft. Seinen For- schungsauftrag führt das AIP im Rahmen von nationalen und internationalen Kooperatio- nen aus. Die Beteiligung am Large Binocular Telescope auf dem Mt Graham in Arizona, dem größten optischen Teleskop der Welt, verdient hierbei besondere Erwähnung. Neben seinen Forschungsarbeiten profiliert sich das Institut zunehmend als Kompetenzzentrum im Bereich der Entwicklung von Forschungstechnologie. Vier gemeinsame Berufungen mit der Universität Potsdam und mehrere außerplanmäßige Professuren und Privatdozenturen an Universitäten in der Region und -
Macrocosmo Nº33
HA MAIS DE DOIS ANOS DIFUNDINDO A ASTRONOMIA EM LÍNGUA PORTUGUESA K Y . v HE iniacroCOsmo.com SN 1808-0731 Ano III - Edição n° 33 - Agosto de 2006 * t i •■•'• bSÈlÈWW-'^Sif J fé . ’ ' w s » ws» ■ ' v> í- < • , -N V Í ’\ * ' "fc i 1 7 í l ! - 4 'T\ i V ■ }'- ■t i' ' % r ! ■ 7 ji; ■ 'Í t, ■ ,T $ -f . 3 j i A 'A ! : 1 l 4/ í o dia que o ceu explodiu! t \ Constelação de Andrômeda - Parte II Desnudando a princesa acorrentada £ Dicas Digitais: Softwares e afins, ATM, cursos online e publicações eletrônicas revista macroCOSMO .com Ano III - Edição n° 33 - Agosto de I2006 Editorial Além da órbita de Marte está o cinturão de asteróides, uma região povoada com Redação o material que restou da formação do Sistema Solar. Longe de serem chamados como simples pedras espaciais, os asteróides são objetos rochosos e/ou metálicos, [email protected] sem atmosfera, que estão em órbita do Sol, mas são pequenos demais para serem considerados como planetas. Até agora já foram descobertos mais de 70 Diretor Editor Chefe mil asteróides, a maior parte situados no cinturão de asteróides entre as órbitas Hemerson Brandão de Marte e Júpiter. [email protected] Além desse cinturão podemos encontrar pequenos grupos de asteróides isolados chamados de Troianos que compartilham a mesma órbita de Júpiter. Existem Editora Científica também aqueles que possuem órbitas livres, como é o caso de Hidalgo, Apolo e Walkiria Schulz Ícaro. [email protected] Quando um desses asteróides cruza a nossa órbita temos as crateras de impacto. A maior cratera visível de nosso planeta é a Meteor Crater, com cerca de 1 km de Diagramadores diâmetro e 600 metros de profundidade. -
Variable Stars
VARIABLE STARS RONALD E. MICKLE Denver, Colorado 80211 ©2001 Ronald E. Mickle ABSTRACT The objective of this paper is to research the causes for variability and identify selected stars within telescope reach. In addition, individual observations of the magnitudes (Mv) of selected variable stars were made and a plan designed for more extensive work on variable stars was developed. Variable stars are stars that vary in brightness. They can range from a thousandth of a magnitude to as much as 20 magnitudes. This range of magnitudes, referred to as amplitude variation, can have periods of variability ranging from a fraction of a second to years. Algol, one of the oldest know variables, was known to ancient astronomers to vary in brightness. Today over 30,000 variable stars are known and catalogued, and thousands more are suspected. Variable stars change their brightness for several reasons. Pulsating variables swell and shrink due to internal forces, while an eclipsing binary will dim when it is eclipsed by its binary companion. (Universe 1999; The Astrophysical Journal) Today measurements of the magnitudes of variable stars are made through visual observations using the naked eye, or instruments such as a charge- coupled device (CCD). The observations made for this paper were reported to the American Association of Variable Star Observers (AAVSO) via their website. The AAVSO website lists variable star organizations in 17 countries to which observations can be reported (AAVSO). 1. IDENTIFICATION OF STAR FIELDS Observations were made from Denver, Colorado, United States. Latitude and longitude coordinates are 40ºN, 105ºW. 1.1. EYEPIECE FIELD-OF-VIEW (FOV) AAVSO charts aid in locating the target variable. -
The Structures and Extents of the Chromospheres of Late-Type Stars
The Structures and Extents of the Chromospheres of Late-type Stars A dissertation submitted to the University of Dublin for the degree of Doctor of Philosophy Neal O´ Riain Trinity College Dublin, September 2015 School of Physics University of Dublin Trinity College Declaration I declare that this thesis has not been submitted as an exercise for a degree at this or any other university and it is entirely my own work. I agree to deposit this thesis in the University's open access institu- tional repository or allow the library to do so on my behalf, subject to Irish Copyright Legislation and Trinity College Library conditions of use and acknowledgement. Name: Neal O´ Riain Signature: ........................................ Date: .......................... Summary The chromosphere is the region of a star, above what is traditionally defined as the stellar surface, from which photons freely escape. As the definition implies, this region is characterised by complexity, non- equilibrium, and specifying its structure is a vastly non-linear, non- local problem. In this work we are concerned with the chromospheres of late-type stars, objects of spectral type K to M, the thermodynamic structure, extent, and heating mechanisms of whose chromospheres are not well understood. We use a number of observational and computa- tional methods in order to gain a detailed quantitative understanding of these chromospheres. We construct a model to compute the mm, thermal bremsstrahlung flux from the chromospheres of late-type objects, based on a number of simplifying assumptions concerning their thermodynamic structure. We compare this model with archival and recent observations, and find that the model is capable of reproducing the observed flux from objects of spectral type K to mid-M in the frequency range 100 GHz { 350 GHz. -
Astronomy Magazine 2012 Index Subject Index
Astronomy Magazine 2012 Index Subject Index A AAR (Adirondack Astronomy Retreat), 2:60 AAS (American Astronomical Society), 5:17 Abell 21 (Medusa Nebula; Sharpless 2-274; PK 205+14), 10:62 Abell 33 (planetary nebula), 10:23 Abell 61 (planetary nebula), 8:72 Abell 81 (IC 1454) (planetary nebula), 12:54 Abell 222 (galaxy cluster), 11:18 Abell 223 (galaxy cluster), 11:18 Abell 520 (galaxy cluster), 10:52 ACT-CL J0102-4915 (El Gordo) (galaxy cluster), 10:33 Adirondack Astronomy Retreat (AAR), 2:60 AF (Astronomy Foundation), 1:14 AKARI infrared observatory, 3:17 The Albuquerque Astronomical Society (TAAS), 6:21 Algol (Beta Persei) (variable star), 11:14 ALMA (Atacama Large Millimeter/submillimeter Array), 2:13, 5:22 Alpha Aquilae (Altair) (star), 8:58–59 Alpha Centauri (star system), possibility of manned travel to, 7:22–27 Alpha Cygni (Deneb) (star), 8:58–59 Alpha Lyrae (Vega) (star), 8:58–59 Alpha Virginis (Spica) (star), 12:71 Altair (Alpha Aquilae) (star), 8:58–59 amateur astronomy clubs, 1:14 websites to create observing charts, 3:61–63 American Astronomical Society (AAS), 5:17 Andromeda Galaxy (M31) aging Sun-like stars in, 5:22 black hole in, 6:17 close pass by Triangulum Galaxy, 10:15 collision with Milky Way, 5:47 dwarf galaxies orbiting, 3:20 Antennae (NGC 4038 and NGC 4039) (colliding galaxies), 10:46 antihydrogen, 7:18 antimatter, energy produced when matter collides with, 3:51 Apollo missions, images taken of landing sites, 1:19 Aristarchus Crater (feature on Moon), 10:60–61 Armstrong, Neil, 12:18 arsenic, found in old star, 9:15 -
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Volume 43 Number 1 JAAVSO 2015 The Journal of the American Association of Variable Star Observers The Curious Case of ASAS J174600-2321.3: an Eclipsing Symbiotic Nova in Outburst? Light curve of ASAS J174600-2321.3, based on EROS-2, ASAS-3, and APASS data. Also in this issue... • The Early-Spectral Type W UMa Contact Binary V444 And • The δ Scuti Pulsation Periods in KIC 5197256 • UXOR Hunting among Algol Variables • Early-Time Flux Measurements of SN 2014J Obtained with Small Robotic Telescopes: Extending the AAVSO Light Curve Complete table of contents inside... The American Association of Variable Star Observers 49 Bay State Road, Cambridge, MA 02138, USA The Journal of the American Association of Variable Star Observers Editor John R. Percy Edward F. Guinan Paula Szkody University of Toronto Villanova University University of Washington Toronto, Ontario, Canada Villanova, Pennsylvania Seattle, Washington Associate Editor John B. Hearnshaw Matthew R. Templeton Elizabeth O. Waagen University of Canterbury AAVSO Christchurch, New Zealand Production Editor Nikolaus Vogt Michael Saladyga Laszlo L. Kiss Universidad de Valparaiso Konkoly Observatory Valparaiso, Chile Budapest, Hungary Editorial Board Douglas L. Welch Geoffrey C. Clayton Katrien Kolenberg McMaster University Louisiana State University Universities of Antwerp Hamilton, Ontario, Canada Baton Rouge, Louisiana and of Leuven, Belgium and Harvard-Smithsonian Center David B. Williams Zhibin Dai for Astrophysics Whitestown, Indiana Yunnan Observatories Cambridge, Massachusetts Kunming City, Yunnan, China Thomas R. Williams Ulisse Munari Houston, Texas Kosmas Gazeas INAF/Astronomical Observatory University of Athens of Padua Lee Anne M. Willson Athens, Greece Asiago, Italy Iowa State University Ames, Iowa The Council of the American Association of Variable Star Observers 2014–2015 Director Arne A. -
Universe of Binaries, Binaries in the Universe
Universe of Binaries, Binaries in the Universe 7-11 September 2019, Telč, Czech Republic Conference venue facility of the Masaryk University Taken from https://www.uct.muni.cz/media/3140349/skladacka_dl_en1_150dpi.pdf Taken from https://www.uct.muni.cz/media/3140349/skladacka_dl_en1_150dpi.pdf Program Friday, September 6 19:00 Welcome drink Saturday, September 7 08:45-09:00 Welcome 09:00-09:40 Kafka Citizen-scientists supporting binary star research 09:40-10:00 Zejda Pro-Am collaboration in stellar astrophysics „Made in Czech Republic“ 10:00-10:40 Kim Professional-amateur programs at Chungbuk National Observatory 10:40-11:00 Coffee/Tea Break 11:00-11:40 Teyssier Symbiotic Binaries Monitoring 11:40-12:00 Olah et al. The importance of studying active giant stars in eclipsing binaries - and the role of citizen scientists in finding them 12:00-12:40 Czismadia From CoRoT to PLATO: large photometric exoplanet space surveys for the planetary and binary star community 12:40-14:00 Lunch 14:00-14:20 Forró EBs hiding in the background: the Kepler Pixel Project 14:20-14:40 Villasenor Multiplicity properties of B-type stars from the B-star Binaries Characterisation Project 14:40-15:00 Rukmini et al. Photometric study of 61 total eclipsing contact binaries from ASAS, OGLE, HATNet, AST3 and TESS databases 15:00-15:20 Hajdu et al. Hierarchical triple star systems towards the Galactic Bulge through the OGLE's eye 15:20-15:40 Christopoulou et al. What we can learn from Eclipsing Binaries in Large Surveys: The case of EA Catalina systems 15:40-16:00 Coffee/Tea Break 16:00-16:20 Stevens & Zhou A Binary of Ice and Fire 16:20-16:40 Lalounta et al. -
Baltic Astronomy, Vol.19, 95–110, 2010 CHEMICAL COMPOSITION
Baltic Astronomy, vol. 19, 95–110, 2010 CHEMICAL COMPOSITION OF THE RS CVn-TYPE STAR LAMBDA ANDROMEDAE G. Tautvaiˇsiene˙1, G. Bariseviˇcius1, S. Berdyugina2, Y. Chorniy1 and I. Ilyin3 1 Institute of Theoretical Physics and Astronomy, Vilnius University, Goˇstauto 12, Vilnius LT-01108, Lithuania 2 Kiepenheuer Institut fur¨ Sonnenphysik, Sch¨oneckstrasse 6, Freiburg D-79104, Germany 3 Astrophysical Institute Potsdam, An der Sternwarte 16, Potsdam D-14482, Germany Received: 2010 June 8; accepted: 2010 June 15 Abstract. Photospheric parameters and chemical composition are deter- mined for the single-lined chromospherically active RS CVn-type star λ And (HD 222107). From the high resolution spectra obtained on the Nordic Optical Telescope, abundances of 22 chemical elements and isotopes, including such key elements as 12C, 13C, N and O, were investigated. The differential line analysis with the MARCS model atmospheres gives Teff = 4830 K, log g = 2.8, [Fe/H] = –0.53, [C/Fe] = 0.09, [N/Fe] = 0.35, [O/Fe] = 0.45, C/N = 2.21, 12C/13C = 14. The 12C/13C ratio for a star of the RS CVn-type is determined for the first time, and its low value gives a hint that extra-mixing processes may start acting in low-mass chromospherically active stars below the bump of the luminosity function of red giants. Key words: stars: RS CVn binaries, abundances – stars: individual (λ And = HD 222107) 1. INTRODUCTION The RS CVn-type stars have been studied thoroughly since 1965 when their peculiar light curves were detected (Rodon´o 1965; Chisari & Lacona 1965) and a new distinct class of binaries was named (Olivier 1974; Hall 1976). -
Extrasolar Planets and Their Host Stars
Kaspar von Braun & Tabetha S. Boyajian Extrasolar Planets and Their Host Stars July 25, 2017 arXiv:1707.07405v1 [astro-ph.EP] 24 Jul 2017 Springer Preface In astronomy or indeed any collaborative environment, it pays to figure out with whom one can work well. From existing projects or simply conversations, research ideas appear, are developed, take shape, sometimes take a detour into some un- expected directions, often need to be refocused, are sometimes divided up and/or distributed among collaborators, and are (hopefully) published. After a number of these cycles repeat, something bigger may be born, all of which one then tries to simultaneously fit into one’s head for what feels like a challenging amount of time. That was certainly the case a long time ago when writing a PhD dissertation. Since then, there have been postdoctoral fellowships and appointments, permanent and adjunct positions, and former, current, and future collaborators. And yet, con- versations spawn research ideas, which take many different turns and may divide up into a multitude of approaches or related or perhaps unrelated subjects. Again, one had better figure out with whom one likes to work. And again, in the process of writing this Brief, one needs create something bigger by focusing the relevant pieces of work into one (hopefully) coherent manuscript. It is an honor, a privi- lege, an amazing experience, and simply a lot of fun to be and have been working with all the people who have had an influence on our work and thereby on this book. To quote the late and great Jim Croce: ”If you dig it, do it.