PPT-Supernova 1987A Progenitor

Original source Arnett WD et al 1989 Supernova 1987A Annual Review of Astronomy and Astrophysics 27 629700 From Wikipedia article downloaded 9814 http enwikipediaorgwikiSN1987A. the excitement continues. Bruno . Leibundgut. ESO. SN 1987A – a great collaboration. Monitoring over the past two and a half decades. Claes. . Fransson. (Stockholm). Bob . Kirshner. (. CfA. ) . . Supernovae . J081659.74+511233.7 . and . J07285387+3349106. . with . the BSU . Observatory. Benjamin . Lombard and Sarah Peck . (Mentor: Professor Jamie Kern). Bridgewater State University. Abstract. Briana Ingermann & Parke Loyd. Meet Pulsational Pair-Instability SN Progenitor. After a short MS life, our progenitor senses something is wrong. A runaway thermonuclear explosion ejects a shell, and our progenitor feels better. Jim Kneller. NC State University. NOW 2010. The neutrinos we will detect from the next SN in our Galaxy will tell us much about the explosion . and. the neutrino.. The flavour content of the signal changes as it propagates from the proto-neutron star to our detectors here on Earth.. (Supernova Impostors) Schuyler Van Dyk IPAC/Caltech USA Supernova Impostors • Observed outburst with ~10 49 - 50 erg, i.e., comparable to that of a SN • Many impostors spectroscopica Arshed A. Quyyumi, MD . Professor of Medicine . Emory Clinical Cardiovascular Research Institute (ECCRI). Emory University School of Medicine. Atlanta, GA. Grant support: . National Institutes of Health, . Laura Chomiuk. Jansky. Fellow, Michigan State University. Supernova Types: I vs. II. Type I:. No Hydrogen. Thermonuclear WD explosions (. Ia. ) . and. . Core collapse of massive stars stripped of H envelopes (. Physics Opportunities with. Supernova Neutrinos. Georg Raffelt, Max-Planck-Institut für Physik, München. Sanduleak -69 202. Sanduleak . -. 69 202. Large Magellanic Cloud . Distance 50 kpc . (160.000 light years). 1. John Beacom, The Ohio State University. 2. Plan of the Talk. Introduction to Supernova . N. eutrinos. Focus on . B. urst . D. etection. . What will we know after the next burst?. What . new capabilities do we need?. Highlights of the past 25 years. Outstanding mysteries and surprises. What we can expect to learn, sooner and later. TOPICS. Supernova Energy Sources. Core collapse: . with WFIRST . DRM1 and DRM2. C Baltay. June 1, 2012. Supernova Surveys . using . Slitless. Spectroscopy. Use Imager for . SNe. discovery and to get . lightcurves. Use . slitless. spectroscopy to type supernovae and get redshifts. Instrument Chemistries for each step in the decontamination process. Pre-cleaning. Manual cleaning. Automated cleaning. Case Solutions. CSR Ink and adhesive remover. SchmutzOff stainless steel, acid based re-conditioner and . Instrument Chemistries for each step in the decontamination process. Pre-cleaning. Manual cleaning. Automated cleaning. © 2010 Case Medical, Inc.. Case Solutions. CSR Ink and adhesive remover. SchmutzOff stainless steel, acid based re-conditioner and . Corresponding author: Review ArticleJournal of Blood & Lymph Journal of Blood & LymphISSN: 2165-7831 Volume 8  Issue 2  1000221J Blood Lymph, an open access journalISSN: 2165-7831 Page 2 of 6 e