LP 622-13 , the SIMBAD biblio

LP 622-13 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST21:33:16

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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
1994BAAS...26..901D 264 ~ Evidence for homogeneous ionization of helium in the local interstellar medium from EUVE spectroscopy of hot DA stars. DUPUIS J., VENNES S., BOWYER S., et al.
1999ApJS..121....1M viz 3047 394 A catalog of spectroscopically identified white dwarfs. McCOOK G.P. and SION E.M.
1999ApJS..123..639N viz 2628 37 A search for stars of very low metal abundance. III. UBV photometry of metal-weak candidates. NORRIS J.E., RYAN S.G. and BEERS T.C.
2004AJ....128.2402L viz 135 16 Abundances of extremely metal-poor star candidates. LAI D.K., BOLTE M., JOHNSON J.A., et al.
2011ApJ...743..138G viz 15       D               2 1365 300 A spectroscopic survey and analysis of bright, hydrogen-rich white dwarfs. GIANNINAS A., BERGERON P. and RUIZ M.T.
2013ApJ...778...56C viz 15       D               1 135 157 Normal and outlying populations of the Milky Way stellar halo at [Fe/H] ←2. COHEN J.G., CHRISTLIEB N., THOMPSON I., et al.
2014ApJ...797...21P viz 15       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.
2016yCat....1.2035M viz 16       D               14271 ~ A Catalogue of Spectroscopically Identified White Dwarfs MCCOOK G.P. and SION E.M.
2022A&A...661A.103M viz 43           X         1 29 11 High-precision chemical abundances of Galactic building blocks. The distinct chemical abundance sequence of Sequoia. MATSUNO T., KOPPELMAN H.H., HELMI A., 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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