Results 61 to 70 of about 7,335,139 (174)
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
The Broad-Line Type Ic Supernoava SN 2007ru: Adding To The Diversity Of Type Ic Supernovae [PDF]
Photometric and spectral evolution of the Type Ic supernova SN 2007ru until around 210 days after maximum are presented. The spectra show broad spectral features due to very high expansion velocity, normally seen in hypernovae.
Gurugubelli, Uday K +4 more
core
IC² Institute Annual Report 2000-2001 [PDF]
Annual report of the IC² Institute (Innovation, Creativity, and Capital) at The University of Texas at Austin. Programs covered include: Austin Technology Incubator; Cross Border Institute for Regional Development (CBIRD); Emerging Texas Economy; IC² ...
IC² Institute
core +1 more source
For over 25 yr, the origin of long-duration gamma-ray bursts (lGRBs) has been linked to the collapse of rotating massive stars. However, we have yet to pinpoint the stellar progenitor powering these transients.
Christopher L. Fryer +7 more
doaj +1 more source
Type Ib/Ic Supernovae: Effect of Nickel Mixing on the Early-time Color Evolution and Implications for the Progenitors [PDF]
We investigate the effect of mixing of radioactive nickel (Ni-56) on the early-time color evolution of Type Ib and Ic supernovae (SNe Ib/Ic) using multigroup radiation hydrodynamics simulations.
Blinnikov, Sergey +4 more
core +1 more source
SN 2022oqm–A Ca-rich Explosion of a Compact Progenitor Embedded in C/O Circumstellar Material
We present the discovery and analysis of SN 2022oqm, a Type Ic supernova (SN) detected
Ido Irani +29 more
doaj +1 more source
SN 2024abup is a nearby broad-lined Type Ic supernova (SN Ic-bl) in NGC 0681 at a distance of 23.3 ± 1.6 Mpc. As energetic explosions of massive stars, SNe Ic-bl are considered a plausible site for rapid-neutron capture nucleosynthesis ( r -process) and ...
Manisha Shrestha +44 more
doaj +1 more source
Observational constraints on the progenitor metallicities of core-collapse supernovae [PDF]
Artículo de publicación ISIWe present constraints on the progenitor metallicities of core-collapse supernovae. To date, nearly all metallicity constraints have been inferred from indirect methods such as metallicity gradients in host galaxies ...
James, P. A. +9 more
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We present 1800 multiwavelength Type Ib/c supernovae light-curve models obtained by running the radiation transport code Sedona and varying the mass distribution, velocity profile, and abundance ejecta profiles of helium star progenitors.
S. Karthik Yadavalli +5 more
doaj +1 more source
88th Annual Meeting of the Meteoritical Society 2026: Abstracts
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley +1 more source

