Pulsational pair-instability supernovae
SE Woosley - The Astrophysical Journal, 2017 - iopscience.iop.org
The final evolution of stars in the mass range 70–140${\text {}}{M} _ {\odot} $ is explored.
Depending upon their mass loss history and rotation rates, these stars will end their lives as …
Depending upon their mass loss history and rotation rates, these stars will end their lives as …
The direct identification of core-collapse supernova progenitors
SD Van Dyk - … Transactions of the Royal Society A …, 2017 - royalsocietypublishing.org
To place core-collapse supernovae (SNe) in context with the evolution of massive stars, it is
necessary to determine their stellar origins. I describe the direct identification of SN …
necessary to determine their stellar origins. I describe the direct identification of SN …
Pre-supernova outbursts via wave heating in massive stars–I. Red supergiants
J Fuller - Monthly Notices of the Royal Astronomical Society, 2017 - academic.oup.com
Early observations of supernovae (SNe) indicate that enhanced mass-loss and pre-SN
outbursts may occur in progenitors of many types of SNe. We investigate the role of energy …
outbursts may occur in progenitors of many types of SNe. We investigate the role of energy …
Observational and physical classification of supernovae
A Gal-Yam - ar** of the Progenitor
H Kuncarayakti, K Maeda, L Dessart… - The Astrophysical …, 2022 - iopscience.iop.org
Supernova (SN) 2021ocs was discovered in the galaxy NGC 7828 (z= 0.01911) within the
interacting system Arp 144 and subsequently classified as a normal Type Ic SN around peak …
interacting system Arp 144 and subsequently classified as a normal Type Ic SN around peak …
A radio-detected type Ia supernova with helium-rich circumstellar material
Abstract Type Ia supernovae (SNe Ia) are thermonuclear explosions of degenerate white
dwarf stars destabilized by mass accretion from a companion star, but the nature of their …
dwarf stars destabilized by mass accretion from a companion star, but the nature of their …
Statistical properties of the nebular spectra of 103 stripped-envelope core-collapse supernovae
We present an analysis of the nebular spectra of 103 stripped-envelope (SE) supernovae
(SNe) collected from the literature and observed with the Subaru Telescope from 2002 to …
(SNe) collected from the literature and observed with the Subaru Telescope from 2002 to …