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 . 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. 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. 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). (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 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 . 0. Topic: . Multiwavelength observations. Concepts: . Infrared observations, X-ray observations, Optical observations, EM spectrum . Missions: . “Great Observatories”: . Hubble, Chandra, Spitzer;. 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). . . . 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!. Surface accuracy not so important, so easy to make large one.. angular resolution . . . wavelength. mirror diameter. D larger than optical case, but wavelength . much. larger (cm's to m's), e.g. for wavelength = 1 cm, diameter = 100 m, resolution = 20".. 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 . Early a ripple a ripple ripple ripple A ripple a rippled 1 a a X X Summary of Ripple Indexes 4 of Variances Between Wavelengths From Different Stratigraphic Units Denominator of Sign

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