Работы, цитирующие эту работу

Работ: 4

Работа: Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range in supernovae environments

1. Violent mergers can explain the inflated state of some of the fastest stars in the Galaxy

   Aakash Bhat, Rüdiger Pakmor, Ken J. Shen +4

   СтатьяAstronomy and Astrophysical ResearchAstronomy and Astrophysics2026Цитирований: 1

   ABIABI:AkademIndex/openalex/2026.article.000159

2. Axisymmetric general relativistic simulations of the accretion-induced collapse of white dwarfs

   Ernazar Abdikamalov, Christian D. Ott, Luciano Rezzolla +4

   СтатьяGamma-ray bursts and supernovaePhysical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology2010Цитирований: 0

   ABIABI:AkademIndex/openalex/2010.article.000024

3. Drawing the line between explosion and collapse in electron-capture supernovae

   Alexander Holas, Samuel Jones, Friedrich K. Röpke +5

   СтатьяGamma-ray bursts and supernovaeAstronomy and Astrophysics2026Цитирований: 0

   ABIABI:AkademIndex/openalex/2026.article.000233

4. Simulations of Interacting Binary Systems—Pathways to Radio-bright Gamma-Ray Burst Progenitors

   Angel Hernandez, Roseanne M. Cheng, Nicole M. Lloyd-Ronning +1

   СтатьяGamma-ray bursts and supernovaeThe Astrophysical Journal2026Цитирований: 0

   ABIABI:AkademIndex/openalex/2026.article.021285