PPT-Superluminous supernovae – constraints on progenitor stars

SJ Smartt M Nicholl C Inserra A Jerkstrand TW Chen M McCrum K Smith D Young Queens University Belfast Not an unbiased review See Handbook of Supernovae Andy Howell Superluminous Supernovae. Soprano I Hence  stars,  you  daz- zle but the sight,   you teach to Soprano II Hence  stars, \r \r \r Alto Hence  stars, hence   stars too  dim of light,  you  daz-  zle  b Original source: Arnett. , W.D.; et al. (1989). "Supernova 1987A". . Annual Review of Astronomy and Astrophysics. . 27. : 629–700. .. From Wikipedia article, downloaded 9/8/14, . http. ://. en.wikipedia.org/wiki/SN_1987A. 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, . . 1. Les régions de formation d’étoiles: du . keV. au . TeV. Atelier CTA. Thierry . Montmerle. Laboratoire d'Astrophysique de Grenoble, France. Les étoiles massives (> . 8 M. a. ): . effets de rétroaction et évolution des associations OB. Array for Sub-. F. ermi . E. nergy . H. eavy Ion . R. eaction . D. ynamics. Summer REU Program 2012. Brittany Abromeit. August 3, 2012. 1. Outline:. Supernovae and the resulting neutron stars. Nuclear Equation of State. Talk by: John McCann. Paper by: D. . Poznanski. , Z. Kostrzewa-Rutkowska, L. Wyrzykowski & N. . Blagorodnova. OGLE-IV. OGLE – Optical Gravitational Lensing Experiment, Phase four. Las . 回転単独星モデルと連星モデル. 梅田　秀之. （東京大学　天文学専攻）. Introduction. (L-)GRB progenitor – . associated with . Hypernovae. . . Massive Stars. Central engine (popular models):. SN2014J. R. Margutti. Harvard . nothing. Margutti 13, 14; . Kamble. 13; . Soderberg. 06, 10. Energy partitioning. SNe. are an OPTICAL . phenomenon. 10. 51. erg. OPTICAL. 10. 47. erg. X-rays/Radio. Developed by . the SOFIA Team. 0. Topic: . Supernovae.. Concepts: . Supernovae, planet formation, infrared observations. Missionb. : . SOFIA. Coordinated by: . the NASA Astrophysics Forum. An Instructor’s Guide for using the slide sets is available at the ASP website . Mysterious explosions in the Universe. Poonam Chandra. Royal Military College of Canada. Universe is 14 billion years old.. Our sun is 5 billion years.. Supernovae and Gamma ray bursts. Explosions lasting fraction of a second to few seconds.. light curves and spectral evolution. Bruno . Leibundgut. ESO. The core-collapse SN poster child. SN 1987A. the best observed supernova ever. Suntzeff. (2003). (also . Fransson. et al. 2007). What do we want to learn about supernovae?. Most stars either have M < 1.4 . M. ʘ. , . or can lose enough mass during post-main sequence evolution to get there, and end as white dwarf. However if core is more massive, nothing can stop gravitational collapse. University of Sheffield. What is a supernova?. Stellar explosions. Types of supernova. The importance of. supernovae. Supernova remnants. Stellar explosions. Most stars are a balancing act between gravity and pressure. axion. -photon . coupling. Oscar . Straniero. . . Italian National Institute of Astrophysics . . and INFN LNGS (Italy). Adrian Ayala. . Granada & Rome Universities (Spain/Italy). Maurizio .