Pop III i-process nucleosynthesis and the elemental abundances of SMSS J0313−6708 and the most iron-poor stars-Reference-Cited by-同舟云学术

Pop III i-process nucleosynthesis and the elemental abundances of SMSS J0313−6708 and the most iron-poor stars

Published:2017-11-23 Issue:1 Volume:474 Page:L37-L41
ISSN:1745-3925
Container-title:Monthly Notices of the Royal Astronomical Society: Letters
language:en
Short-container-title:

Author:

Clarkson O¹²,Herwig F¹²,Pignatari M²³

Affiliation:

1. Department of Physics & Astronomy, University of Victoria, PO Box 3055, Victoria, BC V8W 3P6, Canada

2. Joint Institute for Nuclear Astrophysics, Center for the Evolution of the Elements, Michigan State University, 640 South Shaw Lane, East Lansing, MI 48824, USA

3. E.A. Milne Centre for Astrophysics, University of Hull, Hull, HU6 7RX, UK

Funder

NSF

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnrasl/article-pdf/474/1/L37/24841490/slx190.pdf

Reference37 articles.

1. Chaos and turbulent nucleosynthesis prior to a supernova explosion

2. The Discovery and Analysis of Very Metal-Poor Stars in the Galaxy

3. NUCLEOSYNTHESIS IN A PRIMORDIAL SUPERNOVA: CARBON AND OXYGEN ABUNDANCES IN SMSS J031300.36–670839.3

4. Constraints on CEMP-no progenitors from nuclear astrophysics

5. HE 0107−5240, a Chemically Ancient Star. I. A Detailed Abundance Analysis

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