Results 71 to 80 of about 8,434 (211)
Late-time Optical and X-Ray Emission Evolution of the Oxygen-rich SN 1996cr
When the ejecta of a supernova (SN) interact with the progenitor star's circumstellar environment, a strong shock is driven back into the ejecta, causing the material to become bright optically and in X-rays.
Daniel Patnaude +4 more
doaj +1 more source
Long-term observations of synchrotron emission from supernovae (SNe), covering more than a year after the explosion, provide a unique opportunity to study the poorly understood evolution of massive stars in the final millennium of their lives via changes
Keiichi Maeda +6 more
doaj +1 more source
Type Ibc supernovae in disturbed galaxies: evidence for a top-heavy IMF
We compare the radial locations of 178 core-collapse supernovae to the R-band and H alpha light distributions of their host galaxies. When the galaxies are split into `disturbed' and `undisturbed' categories, a striking difference emerges.
Anderson +31 more
core +1 more source
Optical Spectroscopy of Type Ib/c Supernovae
Accepted for publication in the March issue of AJ.
Matheson, Thomas +4 more
openaire +2 more sources
Evolutionary Models for Type Ib/c Supernova Progenitors [PDF]
AbstractSNe Ib/c mark the deaths of hydrogen-deficient massive stars. The evolutionary scenarios for SNe Ib/c progenitors involve many important physical processes including mass loss by winds and its metallicity dependence, stellar rotation, and binary interactions. This makes SNe Ib/c an excellent test bed for stellar evolution theory.
openaire +2 more sources
ABSTRACT Anthropogenic impact has transitioned from threatening already rare species to causing significant declines in once numerous organisms. Long‐tailed duck (Clangula hyemalis) and velvet scoter (Melanitta fusca) were once important quarry sea duck species in NW Europe, but recent declines resulted in their reclassification as vulnerable on the ...
María I. Cádiz +5 more
wiley +1 more source
We present multiband ATLAS and ZTF photometry for SN 2019tsf, a Type Ib stripped-envelope supernova (SESN). The slow spectral evolution could be associated with an uncommon explosion mechanism specific to this SN.
Yossef Zenati +43 more
doaj +1 more source
Upcoming LIGO–Virgo–KAGRA (LVK) observational runs offer new opportunities to probe the central engines of extreme transient events. Cosmological gamma-ray bursts (GRBs) and core-collapse supernovae (CC-SNe), in particular, are believed to be powered by ...
Maurice H. P. M. van Putten
doaj +1 more source
Swift Observations of X-ray supernovae [PDF]
We present a result of X-ray supernovae (SNe) survey using the Swift satellite public archive. An automatic searching program was designed to search X-ray SNe among all of the Swift archival observations between November 2004 and February 2011. Using the
Li, K. L., Pun, Chun. S. J.
core
Inhomogeneities in type Ib/c supernovae: An inverse Compton scattering origin of the X-ray emission
Inhomogeneities in a synchrotron source can severely affect the conclusions drawn from observations regarding the source properties. However, their presence is not always easy to establish, since several other effects can give rise to similar observed ...
Bjornsson, C. -I.
core +1 more source

