Results 131 to 140 of about 5,709 (225)

Gravitational Waves due to Population III Core Collapse Supernovae

open access: yes, 2012
Faculty Advisor: Professor Vuk MandicMy goal was to examine the accuracy of the claim in Sandick et al (2006) that LIGO would be able to observe Gravitational Waves emitted from the core collapse supernovae of Population III stars.This research was ...
Lovdal, Christopher
core  

87th Annual Meeting of the Meteoritical Society 2025: Abstracts

open access: yes
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley   +1 more source

SN 2017hcc and SN 2023usc—A Comparative Spectroscopic Study of Type IIn Supernovae

open access: yesThe Astrophysical Journal
We report on a spectroscopic study of the bright, nearby type IIn supernovae SN 2017hcc and SN 2023usc using data obtained from the Himalayan Chandra Telescope.
V. Sethulakshmi   +3 more
doaj   +1 more source

A New Mechanism for Gravitational-Wave Emission in Core-Collapse Supernovae [PDF]

open access: yes, 2006
We present a new theory for the gravitational wave signatures of core-collapse supernovae. Previous studies identified axisymmetric rotating core collapse, core bounce, postbounce convection, and anisotropic neutrino emission as the primary processes and
Livne, Eli   +7 more
core  

86th Annual Meeting of the Meteoritical Society (2024)

open access: yes
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley   +1 more source

SN 2024abvb: A Type Icn Supernova in the Outskirts of Its Host Galaxy

open access: yesThe Astrophysical Journal
We present multiband photometric and spectroscopic observations of supernova (SN) 2024abvb, which exhibits early-time prominent photoionized narrow emission lines of C II superposed on a blue continuum.
Maokai Hu   +13 more
doaj   +1 more source

The innermost zones of core collapse supernovae

open access: yes, 2005
We achieve successful explosions (of otherwise non-explosive models) by enhancing the neutrino luminosity in two different ways. The resulting electron fraction Y_e in the innermost ejecta reaches or in some zones even exceeds 0.5.
Hauser, P.   +4 more
core  

Supernova Siblings and Spectroscopic Host Galaxy Properties

open access: yesThe Astrophysical Journal
Over the past century, supernova (SN) searches have detected multiple supernovae (SNe) in hundreds of individual galaxies. So-called SN siblings discovered in the same galaxy present an opportunity to constrain the dependence of the properties of SNe on ...
Laura Salo   +4 more
doaj   +1 more source

Astrophysics with Gravitational Wave Signals from Core-Collapse Supernovae [PDF]

open access: yes, 2019
The next generation of gravitational wave detectors will improve the detection prospects for gravitational waves from core-collapse supernovae. The complex astrophysics involved in core-collapse supernovae pose a significant challenge to modeling such ...
Roma, Vincent
core  

Nucleosynthetic Analysis of Three-dimensional Core-collapse Supernova Simulations

open access: yesThe Astrophysical Journal
We study in detail the ejecta conditions and theoretical nucleosynthetic results for 18 three-dimensional core-collapse supernova (CCSN) simulations done by F ornax .
Tianshu Wang, Adam Burrows
doaj   +1 more source

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