PPT-Early History of Supernovae

S R Kulkarni Caltech Optical Observatories Key Papers On Supernovae Baade amp Zwicky 1934a Cosmic Rays From Supernovae Baade amp Zwicky 1934b On the Search for Supernovae . 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. Super-Luminous Supernovae. Shri. Kulkarni & Robert . Quimby. Caltech, Pasadena. Stellar . Evolution (Old Story). 2. ZAMS Mass (M. o. ). Ending. <8 . C+O. White Dwarf. 8. to 10. Electron Capture -> Neutron Star (:). 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 . The Pre-History of the Philippines . Before Magellan Showed Up. "History of the Philippines." . Wikipedia. . Wikimedia Foundation. Web. 15 Feb. 2016. <https://en.wikipedia.org/wiki/History_of_the_Philippines>.. 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. Chelsea Braun. Credit: Artist illustration ESO, http. ://www.universetoday.com/wp-content/uploads/2006/12/2006-1130supernova.jpg. Overview. What is a Supernova?. Types of Supernovae. Supernovae in NGC 4088. . kings ruled Rome from 600 B.C. to 509 BC . Roman aristocrats overthrew the last Etruscan king in 509 BC. Establish a republic. Regal- 753-509 B.C.E. . Rome is ruled by kings. Republic- 510-27 B.C.E. . and. . . Church. . History. Chapter E. The Early Church. Chapter Summary. The Church is made up of both sinners and saints. . In the midst of struggles, the early Church was formed. . The faith of the early martyrs and saints are models and examples for us today. . Students will learn to:. appreciate the relevance of a theme or historical period to the life and mission of the Church today.. demonstrate knowledge of the key aspects of an important theme or period in the Church history..