MAGNETOROTATIONALLY DRIVEN SUPERNOVAE AS THE ORIGIN OF EARLY GALAXY r -PROCESS ELEMENTS?-Reference-Cited by-同舟云学术

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MAGNETOROTATIONALLY DRIVEN SUPERNOVAE AS THE ORIGIN OF EARLY GALAXY r -PROCESS ELEMENTS?

Published:2012-04-13 Issue:1 Volume:750 Page:L22
ISSN:2041-8205
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Winteler C.,Käppeli R.,Perego A.,Arcones A.,Vasset N.,Nishimura N.,Liebendörfer M.,Thielemann F.-K.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference50 articles.

1. Nucleosynthesis-relevant conditions in neutrino-driven supernova outflows

2. Dynamicalr-process studies within the neutrino-driven wind scenario and its sensitivity to the nuclear physics input

3. Neutron star mergers versus core-collapse supernovae as dominant r-process sites in the early Galaxy

4. Supernova mechanisms

5. Магнитогидро динамическая ротационная модель взрыва сверхновой

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4. The gravitational-wave emission from the explosion of a 15 solar mass star with rotation and magnetic fields;Monthly Notices of the Royal Astronomical Society;2024-07-23

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