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. 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 Remants and Pulsar Wind Nebulae in the Chandra Era. 1. Modeling the Dynamical and Radiative Evolution of a Pulsar Wind Nebula inside a Supernova Remnant. Joseph Gelfand (NYU / NSF). Patrick Slane (CfA), Weiqun Zhang (NYU). 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, . 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. 2013/12/18. Speaker . : Yu-. Hsun. Cheng. Professor: Yosuke Mizuno. Introduction. Supernova remnants(SNR):. . This is . the structure resulting from the explosion of a star in a supernova. . It is formed by that the interactive between interstellar and . 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: . . . . Sumit K. . Sarbadhicary. PITT-PACC, University of Pittsburgh. Team. - . Carles. . Badenes. (Pitt), Laura . Chomiuk. , Daniel Huizenga, Jessica Maldonado (MSU), . Damiano. . Caprioli. (U. Chicago). 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!. Developed by . the SOFIA Team. 0. Topic: . Supernovae. Concepts: . Supernovae, planet formation, infrared observations. Mission: . SOFIA. Coordinated by: . the NASA Astrophysics Forum. An Instructor’s Guide for using the slide sets is available at the ASP website . © 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. 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 . 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.