PPT-EVOLUTIONARY PATH TOWARD THE CORE COLLAPSE SUPERNOVA EXPLOS

Author : alida-meadow | Published Date : 2016-02-26

and Alessandro Chieffi INAF Istituto di Astrofisica Spaziale e Fisica Cosmica Italy alessandrochieffiiasfromainafit Marco Limongi INAF Osservatorio Astronomico

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EVOLUTIONARY PATH TOWARD THE CORE COLLAPSE SUPERNOVA EXPLOS: Transcript

and Alessandro Chieffi INAF Istituto di Astrofisica Spaziale e Fisica Cosmica Italy alessandrochieffiiasfromainafit Marco Limongi INAF Osservatorio Astronomico di Roma ITALY. points in the signal path. If too much gain is applied at any one of these points, distortion will be introduced. To removethe distortion you must reduce the gain of the signal to below clipping leve CO. NeO. Pre-SuperNova. Stage. O. SiS. H. . burning. . shell. He burning shell. T~4.0. ×. 10. 9. K. C burning shell. Ne burning shell. O burning shell. Si burning shell. Fe. 2. Pre-. Supernova. . Where do gold earrings come from?. Goals. Explain why stars evolve off the main sequence.. What happens when they leave the main sequence?. How does mass affect what happens?. How do stars die?. The Main Sequence. 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 (. 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. 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). Vs. . binary star progenitors of Type Ii. b. . Sn. e. Niharika. . Sravan. , . pablo. Marchant and . vicky. . kalogera. time domain big data astronomy . and. supernovae. Plethora of survey projects culminating with the LSST will transform SN science by providing unprecedented insights . 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 . in collapsing phase. ～. towards comprehensive neutrino studies . Waseda. . univ.. . Yamada lab.. D1 Chinami Kato. Collaboration with . S. Yamada(. Waseda. ), H. . Nagakura. . (Caltech), W. . Iwakami. 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. supernovae in LIRGs. Image processing courtesy Mischa Schirmer (Gemini Obs.). Supervisors:. . Stuart Ryder. Richard McDermid. Erik Kool. Macquarie University / AAO. Collaborators: . . Seppo Mattila. 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 . 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?.

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