OBSERVATIONAL CONSTRAINTS ON FIRST-STAR NUCLEOSYNTHESIS. I. EVIDENCE FOR MULTIPLE PROGENITORS OF CEMP-NO STARS-Reference-Cited by-同舟云学术

OBSERVATIONAL CONSTRAINTS ON FIRST-STAR NUCLEOSYNTHESIS. I. EVIDENCE FOR MULTIPLE PROGENITORS OF CEMP-NO STARS

Published:2016-12-05 Issue:1 Volume:833 Page:20
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Yoon Jinmi^ORCID,Beers Timothy C.,Placco Vinicius M.^ORCID,Rasmussen Kaitlin C.,Carollo Daniela,He Siyu,Hansen Terese T.^ORCID,Roederer Ian U.^ORCID,Zeanah Jeff

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/833/i=1/a=20/pdf

Reference129 articles.

1. Carbon-enhanced metal-poor stars: a window on AGB nucleosynthesis and binary evolution

2. Wind Roche-lobe overflow: Application to carbon-enhanced metal-poor stars

3. Carbon-enhanced metal-poor stars: a window on AGB nucleosynthesis and binary evolution

4. Modelling the observed properties of carbon-enhanced metal-poor stars using binary population synthesis

5. How plausible are the proposed formation scenarios of CEMP-r/sstars?

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