2013 June Vol. 50 No 590 1) SOLAR
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Optical and Near-Infrared Observations of SN 2011Dh-The First 100 Days
Astronomy & Astrophysics manuscript no. sn2011dh-astro-ph-v2 c ESO 2018 November 4, 2018 Optical and near-infrared observations of SN 2011dh - The first 100 days. M. Ergon1, J. Sollerman1, M. Fraser2, A. Pastorello3, S. Taubenberger4, N. Elias-Rosa5, M. Bersten6, A. Jerkstrand2, S. Benetti3, M.T. Botticella7, C. Fransson1, A. Harutyunyan8, R. Kotak2, S. Smartt2, S. Valenti3, F. Bufano9; 10, E. Cappellaro3, M. Fiaschi3, A. Howell11, E. Kankare12, L. Magill2; 13, S. Mattila12, J. Maund2, R. Naves14, P. Ochner3, J. Ruiz15, K. Smith2, L. Tomasella3, and M. Turatto3 1 The Oskar Klein Centre, Department of Astronomy, AlbaNova, Stockholm University, 106 91 Stockholm, Sweden 2 Astrophysics Research Center, School of Mathematics and Physics, Queens University Belfast, Belfast, BT7 1NN, UK 3 INAF, Osservatorio Astronomico di Padova, vicolo dell’Osservatorio n. 5, 35122 Padua, Italy 4 Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85741 Garching, Germany 5 Institut de Ciències de l’Espai (IEEC-CSIC), Facultat de Ciències, Campus UAB, E-08193 Bellaterra, Spain. 6 Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan 7 INAF-Osservatorio Astronomico di Capodimonte, Salita Moiariello, 16 80131 Napoli, Italy 8 Fundación Galileo Galilei-INAF, Telescopio Nazionale Galileo, Rambla José Ana Fernández Pérez 7, 38712 Breña Baja, TF - Spain 9 INAF, Osservatorio Astrofisico di Catania, Via Santa Sofia, I-95123, Catania, Italy 10 Departamento de Ciencias Fisicas, Universidad Andres Bello, Av. Republica 252, Santiago, Chile 11 Las Cumbres Observatory Global Telescope Network, 6740 Cortona Dr., Suite 102, Goleta, CA 93117 12 Finnish Centre for Astronomy with ESO (FINCA), University of Turku, Väisäläntie 20, FI-21500 Piikkiö, Finland 13 Isaac Newton Group, Apartado 321, E-38700 Santa Cruz de La Palma, Spain 14 Observatorio Montcabrer, C Jaume Balmes 24, Cabrils, Spain 15 Observatorio de Cántabria, Ctra. -
Kavli IPMU Annual 2014 Report
ANNUAL REPORT 2014 REPORT ANNUAL April 2014–March 2015 2014–March April Kavli IPMU Kavli Kavli IPMU Annual Report 2014 April 2014–March 2015 CONTENTS FOREWORD 2 1 INTRODUCTION 4 2 NEWS&EVENTS 8 3 ORGANIZATION 10 4 STAFF 14 5 RESEARCHHIGHLIGHTS 20 5.1 Unbiased Bases and Critical Points of a Potential ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙20 5.2 Secondary Polytopes and the Algebra of the Infrared ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙21 5.3 Moduli of Bridgeland Semistable Objects on 3- Folds and Donaldson- Thomas Invariants ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙22 5.4 Leptogenesis Via Axion Oscillations after Inflation ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙23 5.5 Searching for Matter/Antimatter Asymmetry with T2K Experiment ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ 24 5.6 Development of the Belle II Silicon Vertex Detector ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙26 5.7 Search for Physics beyond Standard Model with KamLAND-Zen ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙28 5.8 Chemical Abundance Patterns of the Most Iron-Poor Stars as Probes of the First Stars in the Universe ∙ ∙ ∙ 29 5.9 Measuring Gravitational lensing Using CMB B-mode Polarization by POLARBEAR ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ 30 5.10 The First Galaxy Maps from the SDSS-IV MaNGA Survey ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙32 5.11 Detection of the Possible Companion Star of Supernova 2011dh ∙ ∙ ∙ ∙ ∙ ∙ -
GRB 190114C: an Upgraded Legend Arxiv:1901.07505V2 [Astro-Ph.HE] 25 Mar 2019
GRB 190114C: An Upgraded Legend Yu Wang1;2, Liang Li 1, Rahim Moradi 1;2, Remo Ruffini 1;2;3;4;5;6 1ICRANet, P.zza della Repubblica 10, 65122 Pescara, Italy. 2ICRA and Dipartimento di Fisica, Sapienza Universita` di Roma, P.le Aldo Moro 5, 00185 Rome, Italy. 3ICRANet - INAF, Viale del Parco Mellini 84, 00136 Rome, Italy. 4Universite´ de Nice Sophia Antipolis, CEDEX 2, Grand Chateauˆ Parc Valrose, Nice, France. 5ICRANet-Rio, Centro Brasileiro de Pesquisas F´ısicas, Rua Dr. Xavier Sigaud 150, 22290–180 Rio de Janeiro, Brazil. 6ICRA, University Campus Bio-Medico of Rome, Via Alvaro del Portillo 21, I-00128 Rome, Italy. [email protected], [email protected], [email protected], ruffi[email protected] arXiv:1901.07505v2 [astro-ph.HE] 25 Mar 2019 1 Gamma-ray burst (GRB) 190114C first resembles the legendary GRB 130427A: Both are strong sources of GeV emission, exhibiting consistent GeV spectral evolution, and almost identical in detail for the morphology of light-curves in X-ray, gamma-ray and GeV bands, inferring a standard system with differ- ent scales. GRB 190114C is richer than GRB 130427A: a large percentage of ∼ 30% energy is thermal presenting in the gamma-ray prompt emission, mak- ing it as one of the most thermal-prominent GRBs; Moreover, GRB 190114C extends the horizon of GRB research, that for the first time the ultra-high energy TeV emission (> 300 GeV) is detected in a GRB as reported by the MAGIC team. Furthermore, GRB 190114C urges us to revisit the traditional theoretical framework, since most of the GRB’s energy may emit in the GeV and TeV range, not in the conventional MeV range. -
Výroční Zpráva České Astronomické Společnosti 2011
Výroční zpráva České astronomické společnosti 2011 stručná charakteristika V České astronomické společnosti v roce 2011 pracovalo 8 místních poboček (Praha, Západočeská, Východočeská, Jihočeská, Astronomická společnost Most se statutem pobočky, Třebíč, Valašská astronomická společnost se statutem pobočky a Klub astronomů Liberecka), 9 odborných sekcí (Sekce proměnných hvězd a exoplanet, Zákrytová a astrometrická sekce, Sluneční, Přístrojová a optická sekce, Historická, Astronautická, Kosmologická, Sekce pro mládež a Společnost pro meziplanetární hmotu se statutem sekce), dále Odborná skupina pro temné nebe a Terminologická komise. ČAS měla v závěru roku přes 500 individuálních členů a 22 kolektivních členů (o 2 více než v minulém roce), z nichž nejvýznamnější je Astronomický ústav AV ČR. Společnost vydává věstník Kosmické rozhledy, distribuuje členům navíc popularizační časopis Astropis, provozuje informační a popularizační web www.astro.cz pro nejširší veřejnost a vydává prostřednictvím Odboru mediální komunikace AV ČR tisková prohlášení a zprávy z oblasti astronomie a kosmonautiky. Mezi významné činnosti v roce 2011 patřila odborná činnost sekcí, popularizace astronomie, vyhledávání a podpora mladých talentů v podobě Astronomické olympiády, udělení tří cen, ochrana před světelným znečištěním, role národního koordinátora astronomického programu Evropské noci vědců v ČR a provozování Keplerova muzea v Praze. 1 Výroční zpráva České astronomické společnosti za rok 2011 podrobná O společnosti Česká astronomická společnost je dobrovolné sdružení odborných a vědeckých pracovníků v astronomii, amatérských astronomů a zájemců o astronomii z řad veřejnosti. ČAS dbá o rozvoj astronomie v českých zemích a vytváří pojítko mezi profesionálními a amatérskými astronomy. ČAS je sdružena v Radě vědeckých společností a je kolektivním členem Evropské astronomické společnosti. Volené orgány ČAS pracovaly v roce 2011 v tomto složení Výkonný výbor Předseda Ing. -
Luglio – Settembre 2017
Raccolta di Flash news dal sito www.ilcosmo.net Luglio – Settembre 2017 Mappa di tutti gli elementi noti che formano i detriti spaziali intorno alla Terra. Questa raccolta consente l’archiviazione personale di tutte le Flash news comparse sulla homepage del nostro sito nel periodo sopra indicato. Non vi sono ulteriori commenti alle notizie. Sono impaginate in ordine cronologico di uscita. La redazione. Assemblato da Luigi Borghi. Associazione Culturale “Il C.O.S.MO.” (Circolo di Osservazione Scientifico-tecnologica di Modena); C.F.:94144450361 pag: 1 di 50 Questa raccolta, le copie arretrate, i suoi articoli, non possono essere duplicati e commercializzati. È vietata ogni forma di riproduzione, anche parziale, senza l’autorizzazione scritta del circolo “Il C.O.S.Mo”. La loro diffusione all’esterno del circolo e’ vietata. Può essere utilizzata solo dai soci per scopi didattici. - Costo: Gratuito sul WEB per i soci . Raccolta di Flash news dal sito www.ilcosmo.net 1/7/2017 - Il robot che pulirà lo spazio. Sono parecchi anni che gli scienziati e le università di tutto il mondo cercano di risolvere questo enorme problema della sicurezza del volo spaziale: l’accumulo di detriti su orbite operative è potenzialmente devastante per qualsiasi tipo di veicolo spaziale, dai satelliti operativi alle missione con astronauti ed alla ISS. Che non sia un problema facile lo si evince dalla velocità di questi “proiettili” che si aggira sui 28.000 km orari e oltre, dalla impossibilità di identificarne la composizione e dalla impssibilità di determinare i punti di presa di oggetti che, nella maggior parte dei casi, sono pure in rapida rotazione su se stessi. -
MEMORIA IAC 2013 Pero No Todo Son Balances Positivos
MEMORIA 2013 “INSTITUTO DE ASTROFÍSICA DE CANARIAS” EDITA: Unidad de Comunicación y Cultura Científica (UC3) del Instituto de Astrofísica de Canarias (IAC) MAQUETA E IMPRIME: Printisur DEPÓSITO LEGAL: 7- PRESENTACIÓN Índice general 8- CONSORCIO PÚBLICO IAC 12- LOS OBSERVATORIOS DE CANARIAS 14- - Observatorio del Teide (OT) 15- - Observatorio del Roque de los Muchachos (ORM) 16- COMISIÓN PARA LA ASIGNACIÓN DE TIEMPO (CAT) 20- ACUERDOS 22- GRAN TELESCOPIO CANARIAS (GTC) 26- ÁREA DE INVESTIGACIÓN 29- - Estructura del Universo y Cosmología 47- - El Universo Local 80- - Física de las estrellas, Sistemas Planetarios y Medio Interestelar 107- - El Sol y el Sistema Solar 137- - Instrumentación y Espacio 161- - Otros 174- ÁREA DE INSTRUMENTACIÓN 174- - Ingeniería 188- - Producción 192- - Oficina de Proyectos Institucionales y Transferencia de Resultados de Investigación (OTRI) 201- ÁREA DE ENSEÑANZA 201- - Cursos de doctorado 203- - Seminarios científicos 207- - Coloquios 207- - Becas 209- - Tesis doctorales 209- - XXIV Escuela de Invierno: ”Aplicaciones astrofísicas de las lentes gravitatorias” 211- ADMINISTRACIÓN DE SERVICIOS GENERALES 211- - Instituto de Astrofísica 213- - Oficina Técnica para la Protección de la Calidad del Cielo (OTPC) 216- - Observatorio del Teide 216- - Observatorio del Roque de los Muchachos 217- - Centro de Astrofísica de la Palma 218- - Ejecución del Presupuesto 2013 219- GABINETE DE DIRECCIÓN 219- - Ediciones 220- - Carteles 220- - Comunicación y divulgación 232- - Web 234- - Visitas a las instalaciones del IAC 237- -
Monte Carlo Simulations of GRB Afterglows
ABSTRACT WARREN III, DONALD CAMERON. Monte Carlo Simulations of Efficient Shock Acceleration during the Afterglow Phase of Gamma-Ray Bursts. (Under the direction of Donald Ellison.) Gamma-ray bursts (GRBs) signal the violent death of massive stars, and are the brightest ex- plosions in the Universe since the Big Bang itself. Their afterglows are relics of the phenomenal amounts of energy released in the blast, and are visible from radio to X-ray wavelengths up to years after the event. The relativistic jet that is responsible for the GRB drives a strong shock into the circumburst medium that gives rise to the afterglow. The afterglows are thus intimately related to the GRB and its mechanism of origin, so studying the afterglow can offer a great deal of insight into the physics of these extraordinary objects. Afterglows are studied using their photon emission, which cannot be understood without a model for how they generate cosmic rays (CRs)—subatomic particles at energies much higher than the local plasma temperature. The current leading mechanism for converting the bulk energy of shock fronts into energetic particles is diffusive shock acceleration (DSA), in which charged particles gain energy by randomly scattering back and forth across the shock many times. DSA is well-understood in the non-relativistic case—where the shock speed is much lower than the speed of light—and thoroughly-studied (but with greater difficulty) in the relativistic case. At both limits of speed, DSA can be extremely efficient, placing significant amounts of energy into CRs. This must, in turn, affect the structure of the shock, as the presence of the CRs upstream of the shock acts to modify the incoming plasma flow. -
The Deepest Radio Observations of Nearby Type IA Supernovae: Constraining Progenitor Types and Optimizing Future Surveys
Draft version January 20, 2020 Typeset using LATEX default style in AASTeX63 The Deepest Radio Observations of Nearby Type IA Supernovae: Constraining Progenitor Types and Optimizing Future Surveys Peter Lundqvist,1, 2 Esha Kundu,1, 2, 3 Miguel A. Pérez-Torres,4, 5 Stuart D. Ryder,6, 7 Claes-Ingvar Björnsson,1 Javier Moldon,8 Megan K. Argo,8, 9 Robert J. Beswick,8 Antxon Alberdi,4 and Erik C. Kool1, 2, 6, 7 1Department of Astronomy, AlbaNova University Center, Stockholm University, SE-10691 Stockholm, Sweden 2The Oskar Klein Centre, AlbaNova, SE-10691 Stockholm, Sweden 3Curtin Institute of Radio Astronomy, Curtin University, GPO Box U1987, Perth WA 6845, Australia 4Instituto de Astrofísica de Andalucía, Glorieta de las Astronomía, s/n, E-18008 Granada, Spain 5Visiting Scientist: Departamento de Física Teorica, Facultad de Ciencias, Universidad de Zaragoza, Spain 6Dept. of Physics and Astronomy, Macquarie University, Sydney NSW 2109, Australia 7Australian Astronomical Observatory, 105 Delhi Rd, North Ryde, NSW 2113, Australia 8Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, M13 9PL, UK 9Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK (Received December 30, 2019; Revised January 15, 2020; Accepted January 16, 2020) ABSTRACT We report deep radio observations of nearby Type Ia Supernovae (SNe Ia) with the electronic Multi-Element Radio Linked Interferometer Net-work (e-MERLIN), and the Australia Telescope Compact Array (ATCA). No detections were made. With standard assumptions for the energy densities of relativistic electrons going into a power-law energy distribution, and the magnetic field strength (e = B = 0:1), we arrive at the upper limits on mass-loss rate for the progenitor system of SN 2013dy (2016coj, 2018gv, 2018pv, 2019np), to be Û −8 −1 −1 M ∼< 12 ¹2:8; 1:3; 2:1; 1:7º × 10 M yr ¹vw/100 km s º, where vw is the wind speed of the mass loss. -
National Aeronautics and Space Administration Th Ixae Mpacs Ixae Th I
National Aeronautics and Space Administration S pacM e aIX th i This collection of activities is based on a weekly series of space science problems distributed to thousands of teachers during the 2012- 2013 school year. They were intended for students looking for additional challenges in the math and physical science curriculum in grades 5 through 12. The problems were created to be authentic glimpses of modern science and engineering issues, often involving actual research data. The problems were designed to be ‘one-pagers’ with a Teacher’s Guide and Answer Key as a second page. This compact form was deemed very popular by participating teachers. For more weekly classroom activities about astronomy and space visit the NASA website, http://spacemath.gsfc.nasa.gov Add your email address to our mailing list by contacting Dr. Sten Odenwald at [email protected] Front and back cover credits: Front) Grail Gravity Map of the Moon -Grail NASA/ARC/MIT; Dawn Chorus - RBSP/APL/NASA; Erupting Prominence - SDO/NASA; Location of Curiosity - Curiosity/JPL./NASA; Chelyabinsk Meteor - WWW; LL Pegasi Spiral - NASA/ESA Hubble Space Telescope. Back) U Camalopardalis (Courtesy ESA/Hubble, NASA and H. Olofsson (Onsala Space Observatory) Interior Illustrations: All images are courtesy NASA and specific missions as stated on each page, except for the following: 20) Chelyabinsk Meteor and classroom (chelyabinsk.ru); 32) diffraction figure (Wikipedia); 39) Planet accretion (Alan Brandon, Nature magazine, May 2011); 44) Beatrix Mine (J.D. Myers, University of Wyoming); 53) Mars interior (Uncredited ,TopNews.in); 89) Earth Atmosphere (NOAA); 90, 91) Lonely Cloud (Henriette, The Cloud Appreciation Society, 2005); 101, 103) House covered in snow (The Author); This booklet was created through an education grant NNH06ZDA001N- EPO from NASA's Science Mission Directorate. -
JUNE 2013 Volume 40, Number 6
JUNE 2013 Free to members, subscriptions $12 for 12 Volume 40, Number 6 A perennial favorite of the backyard astronomer, Saturn is well-placed for viewing throughout the night. Pat Knoll obtained this image from Kearney Mesa (near San Diego) using a 10-inch LX200 Classic at f/40 using a DFK 21AU618.AS imager. This image was obtained during a full Moon, with moderate sky conditions, in skies as light-polluted as any in Orange County, so Saturn is sure to please no matter what the circumstances. Look for it near the bright star Spica in Virgo about two hours after sunset. OCA CLUB MEETING STAR PARTIES COMING UP The free and open club meeting will The Black Star Canyon site will open on The next session of the Beginners be held June 14 at 7:30 PM in the Ir- June 8. The Anza site will be open on June Class will be held at the Heritage Mu- vine Lecture Hall of the Hashinger Sci- 8. Members are encouraged to check the seum of Orange County at 3101 West ence Center at Chapman University in website calendar for the latest updates on Harvard Street in Santa Ana on June Orange. This month, Mike Simmons star parties and other events. 7. The following class will be held will discuss the global astronomy com- August 2. munity Astronomers Without Borders. Please check the website calendar for the outreach events this month! Volunteers are GOTO SIG: TBA NEXT MEETINGS: July 12, August 9 always welcome! Astro-Imagers SIG: June 18, July 16 Remote Telescopes: TBA You are also reminded to check the web Astrophysics SIG: June 21, July 19 site frequently for updates to the calendar Dark Sky Group: TBA of events and other club news. -
Have You Ever Looked up in Wonder at the Night Sky?
Have you ever looked up in wonder at the night sky? Astronomy is your ultimate stargazing companion, off ering helpful observing tips, gorgeous images, and much more. SPECIAL COLLECTOR’S EDITION n ever mont l issue ou ll n MARCH 2018 I y h y y ’ fi d: • Tips for locating stars, planets, and deep-sky objects. The world’s best-selling astronomy magazine • Monthly sky charts to help you locate observing targets. What Texas astronomers search for Cassini exoplanets • Stunning photos of the most beautiful celestial objects. p. 55 reveals Lowell Observatory’s about Saturn historic • Reviews of the latest telescopes and equipment. refractor • EXPLORING p. 60 the ringed planet p. 20 • Strange stories Celestron of Saturn’s moons CGX Mount p. 28 reviewed p. 64 • Huygens lands on methane- Subscribe Today! soaked Titan p. 48 • Under Cassini’s ONLINE Astronomy.com • CALL 877-246-4835 hood p. 46 Outside the United States and Canada, call 903-636-1125. PLUS Bob Berman on super celestial events p. 8 P33103 Photo Credit: NASA/JPL-Caltech/Space Science Institute ASTRONOMY EXCLUSIVE METEORITE KIT Hold A Space Rock — Or 6 Of Them — In Your Hand! This exclusive Meteorite Kit, developed by meteorite expert Dr. Mike Reynolds, is the ideal way to introduce students and astronomy enthusiasts to iron, stone, and stony-iron meteorites. • 6 meteorite samples, including fragments from Campo del Cielo and Chelyabinsk, Russia. • 3 meteorwrong samples — ordinary rocks often mistaken for meteorites. • 16-page educational booklet, plus a magnet and a lab-type magni er. The kit, packed in a divided storage case, is perfect for classroom use or astronomy enthusiasts. -
Ex-Companions of Supernovae Progenitors Zhichao Xue Louisiana State University and Agricultural and Mechanical College, [email protected]
Louisiana State University LSU Digital Commons LSU Doctoral Dissertations Graduate School 2017 Ex-companions of Supernovae Progenitors Zhichao Xue Louisiana State University and Agricultural and Mechanical College, [email protected] Follow this and additional works at: https://digitalcommons.lsu.edu/gradschool_dissertations Part of the Physical Sciences and Mathematics Commons Recommended Citation Xue, Zhichao, "Ex-companions of Supernovae Progenitors" (2017). LSU Doctoral Dissertations. 4456. https://digitalcommons.lsu.edu/gradschool_dissertations/4456 This Dissertation is brought to you for free and open access by the Graduate School at LSU Digital Commons. It has been accepted for inclusion in LSU Doctoral Dissertations by an authorized graduate school editor of LSU Digital Commons. For more information, please [email protected]. EX-COMPANIONS OF SUPERNOVAE PROGENITORS ADissertation Submitted to the Graduate Faculty of the Louisiana State University and Agricultural and Mechanical College in partial fulfillment of the requirements for the degree of Doctor of Philosophy in The Department of Physics and Astronomy by Zhichao Xue B.S., Shandong University, P.R.China, 2012 July 2017 For Mom and Dad ii Acknowledgements Ihavebeenextremelyfortunatetogainhelp,mentorship,encourageandsupportfrommany incredible people during my pursuit of my Ph.D. I would like to start by thanking my parents for backing up my decision to study abroad alone in the first place despite that I am their only child. Their combined love and support carried me through all the low and high in this process. On an equal level, I would like to express my gratitude to my advisor, Bradley Schaefer. I remembered the first time we met on the day of Christmas eve, 2012 and we talked about astronomy for a straight 6 hours.