UCAC4 481-002020 , the SIMBAD biblio

UCAC4 481-002020 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST20:03:03

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2008ApJ...678.1351A 1 27 106 Carbon-enhanced metal-poor stars. III. Main-sequence turnoff stars from the SDSS SEGUE sample. AOKI W., BEERS T.C., SIVARANI T., et al.
2008AJ....136.2070A viz 15       D               1 128 221 The SEGUE stellar parameter pipeline. III. Comparison with high-resolution spectroscopy of SDSS/SEGUE field stars. ALLENDE PRIETO C., SIVARANI T., BEERS T.C., et al.
2009ApJ...698.1963R 37           X         1 57 66 The end of nucleosynthesis: production of lead and thorium in the early galaxy. ROEDERER I.U., KRATZ K.-L., FREBEL A., et al.
2012ApJ...744..195C 93       D       C       3 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.
2012ApJ...751...14M 50 38 Lithium abundances in carbon-enhanced metal-poor stars. MASSERON T., JOHNSON J.A., LUCATELLO S., et al.
2012MNRAS.422..849B 320       D S   X C F     6 97 85 The s-process in low-metallicity stars - III. Individual analysis of CEMP-s and CEMP-s/r with asymptotic giant branch models. BISTERZO S., GALLINO R., STRANIERO O., et al.
2013AJ....145...13A viz 15       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.
2012A&A...548A..34A viz 15       D               4 134 38 Elemental abundances and classification of carbon-enhanced metal-poor stars. ALLEN D.M., RYAN S.G., ROSSI S., et al.
2013ApJ...765..156C viz 15       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 16       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.
2013RAA....13..313X 15       D               1 22 2 Extremely metal-poor star candidates in the SDSS. XU S.-Y., ZHANG H.-W. and LIU X.-W.
2014ApJ...788..180C viz 15       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 15       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.
2015AJ....149...39A 16       D               4 24 7 High-resolution spectroscopy of extremely metal-poor stars from SDSS/SEGUE. II. Binary fraction. AOKI W., SUDA T., BEERS T.C., et al.
2016A&A...591A.118S viz 16       D               1 31408 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.
2018MNRAS.475.2480P viz 16       D               2 1459 13 The sdA problem - I. Physical properties. PELISOLI I., KEPLER S.O. and KOESTER D.
2019A&A...632A..62C 81             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.
2020ApJ...894...34D viz 16       D               1 24035 ~ The metallicity gradient and complex formation history of the outermost halo of the Milky Way. DIETZ S.E., YOON J., BEERS T.C., et al.
2022ApJS..259...60R viz 17       D               1 139 22 SEGUE-2: Old Milky Way Stars Near and Far. ROCKOSI C.M., SUN LEE Y., MORRISON H.L., et al.
2023ApJ...947...23Z viz 17       D               1 647 14 Chemodynamically Tagged Groups of CEMP Stars in the Halo of the Milky Way. I. Untangling the Origins of CEMP-s and CEMP-no Stars. ZEPEDA J., BEERS T.C., PLACCO V.M., et al.

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