Results 121 to 130 of about 426,951 (145)

First stars X. The nature of three unevolved carbon-enhanced metal-poor stars

open access: yes, 2006
International audienceContext: .On the order of 20% of the very metal-poor stars in the Galaxy exhibit large carbon enhancements. It is important to establish which astrophysical sites and processes are responsible for the elemental abundance patterns of
François, P.   +40 more
core   +1 more source

Probing the first generations of massive stars through fluorine in CEMP-no stars

open access: yesThe European Physical Journal A
We investigate whether the first discovered fluorine-rich CEMP-no star, CS 29498$-$043, can be explained by a very metal-poor rotating massive star. We consider single rotating stellar models of 20 $M_{\odot}$ at a metallicity of $Z = 10^{-5}$, exploring initial rotation rates from $\upsilon_{\rm ini}/\upsilon_{\rm crit} = 0$ to $0.7$ in increments of $
Arthur Choplin, Georges Meynet
openaire   +2 more sources

i process and CEMP-s+r stars [PDF]

open access: yesProceedings of XIII Nuclei in the Cosmos — PoS(NIC XIII), 2015
Christian Ritter   +12 more
openaire   +1 more source

Identifying Risk: Concurrent Overlap of the Antarctic Krill Fishery with Krill-Dependent Predators in the Scotia Sea. [PDF]

open access: yesPLoS One, 2017
Hinke JT   +5 more
europepmc   +1 more source

Detailed analyses of three neutron-capture-rich carbon-enhanced metal-poor stars

open access: yes, 2009
International audienceApproximately 20% of very metal-poor stars ([Fe/H] 1.0). Such stars are referred to as carbon-enhanced metal-poor (CEMP) stars. We present a chemical abundance analysis based on high resolution spectra acquired with UVES at the VLT
Sbordone, Luca   +5 more
core  

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