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The first stars: a classification of CEMP-no stars [PDF]
Astronomy and Astrophysics, 2015 Aims. We propose and apply a new classification for the CEMP–no stars, which are carbon-enhanced metal-poor stars with no overabundance of s-elements and with [Fe/H] generally ≤−2.5. Methods.
André Maeder
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The first stars: CEMP-no stars and signatures of spinstars [PDF]
Astronomy and Astrophysics, 2015 Aims. The CEMP-no stars are “carbon-enhanced-metal-poor” stars that in principle show no evidence of s- and r-elements from neutron captures. We try to understand the origin and nucleosynthetic site of their peculiar CNO, Ne–Na, and Mg–Al abundances.
André Maeder, Cristina Chiappini
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A NEW CEMP-s RR LYRAE STAR [PDF]
Astrophysical Journal Letters, 2012 We show that SDSS J170733.93+585059.7 (hereafter SDSS J1707+58), previously identified by Aoki and collaborators as a carbon-enhanced metal-poor star (with s-process-element enhancements; CEMP-s), on the assumption that it is a main-sequence turn-off star, is the RR Lyrae star VIII-14 identified by the Lick Astrograph Survey.
Kinman, T. D. +3 more
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i-Process nucleosynthesis: Observational evidences from CEMP stars [PDF]
Journal of Astrophysics and Astronomy, 2020 8 pages, 2 figures, accepted for publication in Journal of Astrophysics and Astronomy (JAA)
Aruna Goswami, Partha Pratim Goswami
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CEMP stars: possible hosts to carbon planets in the early Universe [PDF]
Monthly Notices of the Royal Astronomical Society, 2016 11 pages, 5 figures; accepted to ...
Abraham Loeb
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High-resolution spectroscopic observations of the new CEMP-s star CD −50°776
Monthly Notices of the Royal Astronomical Society, 2017Fernando Roig, C B Pereira, N A Drake
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CARBON-ENHANCED METAL-POOR STARS: CEMP-s and CEMP-no SUBCLASSES IN THE HALO SYSTEM OF THE MILKY WAY
Astrophysical Journal, 2014Ken Freeman +2 more
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Are some CEMP-s stars the daughters of spinstars?
Astronomy and Astrophysics, 2017Arthur Choplin, Sylvia Ekström
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How plausible are the proposed formation scenarios of CEMP-r/s stars?
Astronomy and Astrophysics, 2016Carlo Abate, Zheng-Wei Liu
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Astrophysical Journal, 2023 We construct a sample of 644 carbon-enhanced metal-poor (CEMP) stars with abundance analyses based on moderate- to high-resolution spectroscopic studies.
Joseph Zepeda +9 more
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