BPS CS 22944-0039 , the SIMBAD biblio

BPS CS 22944-0039 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST23:06:21

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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
1991ApJS...76.1001P viz 1762 52 Photoelectric UBV photometry of stars selected in the HK objective-prism survey. PRESTON G.W., SHECTMAN S.A. and BEERS T.C.
1992AJ....103.1987B viz 1024 532 A search for stars of very low metal abundance. II. BEERS T.C., PRESTON G.W. and SHECTMAN S.A.
1995ApJS...96..175B viz 1810 175 Kinematics of metal-poor stars in the Galaxy. BEERS T.C. and SOMMER-LARSEN J.
2000AJ....119.2866B viz 2011 171 Kinematics of metal-poor stars in the Galaxy. II. Proper motions for a large nonkinematically selected sample. BEERS T.C., CHIBA M., YOSHII Y., et al.
2006AJ....132...85P viz 61 80 Atmospheres, chemical compositions, and evolutionary histories of very metal-poor red horizontal-branch stars in the galactic field and in NGC 7078 (M15). PRESTON G.W., SNEDEN C., THOMPSON I.B., et al.
2010AJ....140.1694F viz 15       D               7 58 32 The chemical compositions of non-variable red and blue field horizontal branch stars. FOR B.-Q. and SNEDEN C.
2014A&A...571A..62C 39           X         1 44 3 Chemical abundances of the metal-poor horizontal-branch stars BPS CS 22186-005. CALISKAN S., CAFFAU E., BONIFACIO P., et al.
2014ApJ...797...21P viz 16       D               2 606 226 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.
2021ApJ...907...10L viz 17       D               1 1549 37 Dynamically tagged groups of very metal-poor halo stars from the HK and Hamburg/ESO surveys. LIMBERG G., ROSSI S., BEERS T.C., et al.
2021ApJ...914...10C viz 17       D               1 266 18 On the use of field RR Lyrae as galactic probes. III. The α-element abundances. CRESTANI J., BRAGA V.F., FABRIZIO M., et al.

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