PROBING FINAL STAGES OF STELLAR EVOLUTION WITH X-RAY OBSERVATIONS OF SN 2013ej

ABSTRACT Massive stars shape their surroundings with mass loss from winds during their lifetimes. Fast ejecta from supernovae (SNe), from these massive stars, shock this circumstellar medium. Emission generated by this interaction provides a window into the final stages of stellar evolution, by prob...

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Veröffentlicht in:	The Astrophysical journal 2016-01, Vol.817 (1), p.22
Hauptverfasser:	Chakraborti, Sayan, Ray, Alak, Smith, Randall, Margutti, Raffaella, Pooley, David, Bose, Subhash, Sutaria, Firoza, Chandra, Poonam, Dwarkadas, Vikram V., Ryder, Stuart, Maeda, Keiichi
Format:	Artikel
Sprache:	eng
Schlagworte:	ABSORPTION ASTROPHYSICS, COSMOLOGY AND ASTRONOMY circumstellar matter COMPTON EFFECT COMPUTERIZED SIMULATION COSMIC RADIATION Density Ejecta ELECTRONS EMISSION INTERSTELLAR SPACE MASS TRANSFER Massive stars Progenitors (astrophysics) RELATIVISTIC RANGE SHOCK WAVES STAR EVOLUTION stars: mass-loss Stellar evolution STELLAR WINDS SUPERNOVAE supernovae: individual (SN 2013ej) X RADIATION X-rays X-rays: general
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