Neutrino cooling rates due to nickel isotopes for presupernova evolution of massive stars-Reference-Cited by-同舟云学术

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Neutrino cooling rates due to nickel isotopes for presupernova evolution of massive stars

Published:2019-08 Issue: Volume:71 Page:12-24
ISSN:1384-1076
Container-title:New Astronomy
language:en
Short-container-title:New Astronomy

Author:

Nabi Jameel-Un,Shehzadi Ramoona,Majid Muhammad

Funder

Higher Education Commission Pakistan

Pakistan Science Foundation

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics,Instrumentation

Reference48 articles.

1. The Nubase2012 evaluation of nuclear properties

2. Search for important weak interaction nuclei in presupernova evolution

3. Importance of (n,p) reactions for stellar beta decay rates

4. Equation of state in the gravitational collapse of stars

5. Supernova mechanisms

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. A systematic study of super-Eddington layers in the envelopes of massive stars;Astronomy & Astrophysics;2022-12

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