Abundances of carbon-enhanced metal-poor stars as constraints on their formation

C. J. Hansen; Birgitta Nordström; T. T. Hansen; Ryan C Kennedy; V. M. Placco; T. C. Beers; Johannes Andersen; G. Cescutti; C. Chiappini

doi:10.1051/0004-6361/201526895

Abundances of carbon-enhanced metal-poor stars as constraints on their formation

C. J. Hansen, Birgitta Nordström, T. T. Hansen, Ryan C Kennedy, V. M. Placco, T. C. Beers, Johannes Andersen, G. Cescutti, C. Chiappini

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31 Citationer (Scopus)

Originalsprog	Engelsk
Artikelnummer	A37
Tidsskrift	Astronomy & Astrophysics
Vol/bind	588
ISSN	1432-0746
DOI	https://doi.org/10.1051/0004-6361/201526895
Status	Udgivet - 1 apr. 2016

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10.1051/0004-6361/201526895

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title = "Abundances of carbon-enhanced metal-poor stars as constraints on their formation",

keywords = "stars: abundances, stars: Population II, stars: carbon, nuclear reactions, nucleosynthesis, abundances, stars: chemically peculiar",

author = "Hansen, {C. J.} and Birgitta Nordstr{\"o}m and Hansen, {T. T.} and Kennedy, {Ryan C} and Placco, {V. M.} and Beers, {T. C.} and Johannes Andersen and G. Cescutti and C. Chiappini",

year = "2016",

month = apr,

day = "1",

doi = "10.1051/0004-6361/201526895",

language = "English",

volume = "588",

journal = "Astronomy & Astrophysics",

issn = "1432-0746",

publisher = "E D P Sciences",

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TY - JOUR

T1 - Abundances of carbon-enhanced metal-poor stars as constraints on their formation

AU - Hansen, C. J.

AU - Nordström, Birgitta

AU - Hansen, T. T.

AU - Kennedy, Ryan C

AU - Placco, V. M.

AU - Beers, T. C.

AU - Andersen, Johannes

AU - Cescutti, G.

AU - Chiappini, C.

PY - 2016/4/1

Y1 - 2016/4/1

KW - stars: abundances

KW - stars: Population II

KW - stars: carbon

KW - nuclear reactions, nucleosynthesis, abundances

KW - stars: chemically peculiar

U2 - 10.1051/0004-6361/201526895

DO - 10.1051/0004-6361/201526895

M3 - Journal article

SN - 1432-0746

VL - 588

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

M1 - A37

ER -

Abundances of carbon-enhanced metal-poor stars as constraints on their formation

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