SDSS J072352.20+363757.2 , the SIMBAD biblio

SDSS J072352.20+363757.2 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST09:25:46


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Title First 3 Authors
2012ApJ...744..195C 16       D               1 35 134 Carbon-enhanced metal-poor stars in the inner and outer halo components of the Milky Way. CAROLLO D., BEERS T.C., BOVY J., et al.
2013AJ....145...13A viz 16       D               1 151 146 High-resolution spectroscopy of extremely metal-poor stars from SDSS/SEGUE. I. Atmospheric parameters and chemical compositions. AOKI W., BEERS T.C., LEE Y.S., et al.
2013ApJ...765..156C viz 16       D               1 26 2 The CH(G) index as a new criterion for selecting red giant stars. CHEN Y.Q., ZHAO G., CARRELL K., et al.
2013AJ....146..132L 17       D               1 39 128 Carbon-enhanced metal-poor stars in SDSS/SEGUE. I. Carbon abundance estimation and frequency of CEMP stars. LEE Y.S., BEERS T.C., MASSERON T., et al.
2014ApJ...788..180C viz 16       D               1 329 52 Carbon-enhanced metal-poor stars: CEMP-s and CEMP-no subclasses in the halo system of the Milky Way. CAROLLO D., FREEMAN K., BEERS T.C., et al.
2014ApJ...797...21P viz 16       D               1 606 226 Carbon-enhanced metal-poor star frequencies in the galaxy: corrections for the effect of evolutionary status on carbon abundances. PLACCO V.M., FREBEL A., BEERS T.C., et al.
2016A&A...591A.118S viz 16       D               1 31406 141 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2016ApJ...833...20Y viz 16       D               1 304 147 Observational constraints on first-star nucleosynthesis. I. Evidence for multiple progenitors of CEMP-no stars. YOON J., BEERS T.C., PLACCO V.M., et al.
2019MNRAS.490.2241A viz 184       D       C F     3 1012 50 The Pristine survey - VI. The first three years of medium-resolution follow-up spectroscopy of Pristine EMP star candidates. AGUADO D.S., YOUAKIM K., GONZALEZ HERNANDEZ J.I., et al.
2019A&A...632A..62C 84             C       2 261 ~ Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars. CHOPLIN A., TOMINAGA N. and ISHIGAKI M.N.

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