TOMOGRAPHY OF MASSIVE STARS FROM CORE COLLAPSE TO SUPERNOVA SHOCK BREAKOUT
Authors:
- Hasan YükselHYHasan Yüksel
- 6 November 2013
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 778 (1)
Abstract
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This publication has 58 references indexed in Scilit:
- SUPERNOVA NEUTRINO LIGHT CURVES AND SPECTRA FOR VARIOUS PROGENITOR STARS: FROM CORE COLLAPSE TO PROTO-NEUTRON STAR COOLINGThe Astrophysical Journal Supplement Series, 2013
- An outburst from a massive star 40 days before a supernova explosionNature, 2013
- THE LOS ALAMOS SUPERNOVA LIGHT-CURVE PROJECT: COMPUTATIONAL METHODSThe Astrophysical Journal Supplement Series, 2013
- SEEKING COUNTERPARTS TO ADVANCED LIGO/Virgo TRANSIENTS WITHSWIFTThe Astrophysical Journal, 2012
- Diffuse supernova neutrinos: oscillation effects, stellar cooling and progenitor mass dependenceJournal of Cosmology and Astroparticle Physics, 2012
- NON-RELATIVISTIC RADIATION MEDIATED SHOCK BREAKOUTS. II. BOLOMETRIC PROPERTIES OF SUPERNOVA SHOCK BREAKOUTThe Astrophysical Journal, 2012
- IceCube sensitivity for low-energy neutrinos from nearby supernovaeAstronomy & Astrophysics, 2011
- SHOCK BREAKOUT IN TYPE II PLATEAU SUPERNOVAE: PROSPECTS FOR HIGH-REDSHIFT SUPERNOVA SURVEYSThe Astrophysical Journal Supplement Series, 2011
- EARLY SUPERNOVAE LIGHT CURVES FOLLOWING THE SHOCK BREAKOUTThe Astrophysical Journal, 2010
- Supernova neutrinosThe Astrophysical Journal, 1988