Results 91 to 100 of about 8,434 (211)
Searching for Wolf-Rayet Stars in M101
Wolf-Rayet (WR) stars are the evolved descendants of massive O-type stars and are considered to be progenitor candidates for Type Ib/c core-collapse supernovae (SNe).
Bibby, J. L. +5 more
core +1 more source
Multiphase Shock Cooling Emission in Ultrastripped Supernovae
Ultrastripped and Type Ibn supernovae (USSNe and SNe Ibn, respectively) are fast-evolving, hydrogen-poor transients that often show signs of interaction with dense circumstellar material (CSM). S. C. Wu & J.
Annastasia Haynie +3 more
doaj +1 more source
Direct Analysis of Spectra of Type Ib Supernovae [PDF]
Synthetic spectra generated with the parameterized supernova synthetic-spectrum code SYNOW are compared to photospheric-phase spectra of Type Ib supernovae (SNe Ib). Although the synthetic spectra are based on many simplifying approximations, including spherical symmetry, they account well for the observed spectra.
David Branch +16 more
openaire +3 more sources
While about 20 type II supernova (SN II) progenitors have been identified using optical data from the Hubble Space Telescope (HST), direct detection of type Ib/Ic supernova (SN Ib/Ic) progenitors remains challenging, due to their faint optical brightness
Moo-Keon Jung, Sung-Chul Yoon
doaj +1 more source
OBSERVATIONAL PROPERTIES OF TYPE Ib/c SUPERNOVA PROGENITORS IN BINARY SYSTEMS [PDF]
14 pages, 7 figures, 3 tables, accepted for publication in ...
Kim, Hyun-Jeong +2 more
openaire +2 more sources
The nature of Long-GRB host galaxies from chemical abundances
Gamma-ray bursts (GRBs) are the most energetic events after the Big Bang and they have been observed up to very high redshift. By means of measures of chemical abundances now available for the galaxies hosting such events,thought to originate from the ...
Akerman +76 more
core +1 more source
Spectropolarimetric Evolution Reveals Dual-axis Ejecta in the Atypical Magnetar-powered SN 2012au
We present six epochs of optical spectropolarimetric observations of the unique and slow-evolving Type Ib supernova (SN) 2012au, between 0 and 295 day post- R -band maximum.
Sabrina DeSoto +9 more
doaj +1 more source
A White Dwarf Merger Paradigm for Supernovae and Gamma-Ray Bursts
Gamma-ray bursts can appear to be a hundred times as luminous as supernovae, but their underlying energy source(s) have remained a mystery. However, there has been evidence for some time now of an association of gamma-ray bursts with supernovae of Type ...
Middleditch, John
core +2 more sources
Eruptive mass loss of massive stars prior to supernova (SN) explosion is key to understanding their evolution and end fate. An observational signature of pre-SN mass loss is the detection of an early, short-lived peak prior to the radioactive-powered ...
Kaustav K. Das +36 more
doaj +1 more source
We study properties of early radio emission from stripped-envelope supernovae (those of type IIb/Ib/Ic). We suggest there is a sub-class of stripped-envelope supernovae in their radio properties, including optically well-studied type Ic supernovae (SNe ...
Maeda, Keiichi
core +1 more source

