PPT-Insights from Radio Wavelengths into Supernova Progenitor

Author : tatyana-admore | Published Date : 2016-07-23

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

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Insights from Radio Wavelengths into Supernova Progenitor: Transcript

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 . S.P. Reynolds et al.. Martin, Tseng Chao . Hsiung. 2013/12/18. Which contents I will cover…. Shell Supernova Remnants: Obliquity Dependence, and . Summary!. Magnetic Fields in Pulsar-Wind Nebulae.. 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. 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, . 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 . There’s a whole lot of light out there!. The Electromagnetic Spectrum. The electro-magnetic spectrum is made up of visible and . nonvisible. light.. Electromagnetic waves are produced by stars and galaxies.. 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?. 0. Topic: . Multiwavelength. observations. Concepts: . Infrared observations, X-ray observations, Optical observations, EM spectrum . Missions: . “Great Observatories”: . Hubble, Chandra, Spitzer;. 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 . LANDSCAPE. A mass medium delivering audio content to passionate and loyal listeners across multiple platforms. RADIO. RADIO TODAY. RADIO. IT’S ON.. Radio’s incredible reach. RADIO BOASTS HIGHEST MASS REACH . 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 . Radiation and Law of Reflection. Chapter 18:2. And Chapter 19.1 page 570. Electromagnetic Spectrum. Today . we know that there is a full range of electromagnetic radiation known as the . electromagnetic spectrum.

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