PDF-SN Theory and NucleosynthesisSeattle, July 16, 2004Type Ia Supernova T

T Plewa A C Calder DQL N Vladimirova O E B Messer J W Truran E F BrownASCAlliance University of Chicago Flash Center FlashCapabilities Span A Broad Range133 RichtmyerMeshkovinsta. Session Objectives. During this session you will learn the following items:. What is STEM?. What is the BSA response?. What are “Counselors” and “Mentors”?. How will the Old North State Council become “STEM-focused”?. 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. (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 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. Estimates by C. Baltay. DRM 1 compared to IDRM. M. ain . differences as far as Supernovae are concerned:. Larger area Imager. Longer wavelength limit (2.5 microns . vs. 2.0). DRM 1 has same . dia. mirror (1.3 m), DRM 1a has 1.2 m mirror. 21.1 Life after Death for White Dwarfs. 21.2 The End of a High-Mass Star. 21.3 Supernovae. Supernova 1987A. 21.4 The Formation of the Elements. 21.5 The Cycle of Stellar Evolution. Units of Chapter 21. N. eutron . Stars Foreseen. . Supernova . End Products?. When a . supernova. goes off, we can speculate that:. The star might blow itself to smithereens, . scattering all its material into space and leaving . NOVA Counselor and . SUPERNOVA Mentor Training. Introduction. This course is intended to provide potential Nova Counselors and Supernova Mentors with the basic information they need to assist Scouts in completing the requirements to earn the Nova and Supernova awards.. 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: . What is a supernova?. AND NOW. …. A SUPERNOVA IS A STAR THAT INCREASES IN BRIGHTNESS BECAUSE IT’S MASS IS EXPLODING(AWESOME!!!!!!) . HOW . HOT. . IS. . A. . SUPERNOVA. ?. Supernovae can get up to 100 billion degrees Fahrenheit! That is like1 billion suns and possibly more!. supernovae in LIRGs. Image processing courtesy Mischa Schirmer (Gemini Obs.). Supervisors:. . Stuart Ryder. Richard McDermid. Erik Kool. Macquarie University / AAO. Collaborators: . . Seppo Mattila. © 2010 Case Medical, Inc.. Why choose Case Medical’s instrument chemistries?. Super concentrated and ready-to-use cleaners for each step in the decontamination process. Environmentally-friendly with no added dyes, perfumes, fillers or masking agents. 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. © 2010 Case Medical, Inc.. Why choose Case Medical’s instrument chemistries?. Super concentrated and ready-to-use cleaners for each step in the decontamination process. Environmentally-friendly with no added dyes, perfumes, fillers or masking agents.