[ITAL][CLC]r[/CLC][/ITAL]-Process Nucleosynthesis in Neutrino-driven Winds from a Typical Neutron Star with [ITAL]M[/ITAL] = 1.4 [ITAL]M[/ITAL][TINF]⊙[/TINF]-Reference-Cited by-同舟云学术

[ITAL][CLC]r[/CLC][/ITAL]-Process Nucleosynthesis in Neutrino-driven Winds from a Typical Neutron Star with [ITAL]M[/ITAL] = 1.4 [ITAL]M[/ITAL][TINF]⊙[/TINF]

Published:2002-10-20 Issue:2 Volume:578 Page:L137-L140
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:

Author:

Terasawa M.,Sumiyoshi K.,Yamada S.,Suzuki H.,Kajino T.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference29 articles.

1. The mass of the neutron star in Vela X-1

2. On the Formation of Low-Mass Black Holes in Massive Binary Stars

3. Geometry and pulse profiles of x-ray pulsars: Asymmetric relativistic FITS to 4U1538 - 52 and VELA x-1

4. A New Algorithm for Supernova Neutrino Transport and Some Applications

5. Measurement of stellar age from uranium decay

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