HE 1353-2735 , the SIMBAD biblio

HE 1353-2735 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST14:39:48

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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
2000A&A...364L...6D 59   K A   O           4 12 Abundance analysis of two extremely metal-poor stars from the Hamburg/ESO Survey. DEPAGNE E., HILL V., CHRISTLIEB N., et al.
2001A&A...373..159C viz 14       D               3320 239 Catalogue of [Fe/H] determinations for FGK stars: 2001 edition. CAYREL DE STROBEL G., SOUBIRAN C. and RALITE N.
2005ApJ...626..446R viz 211 174 The effective temperature scale of FGK stars. I. Determination of temperatures and angular diameters with the infrared flux method. RAMIREZ I. and MELENDEZ J.
2007A&A...462..851B 2 35 213 First stars. VII - Lithium in extremely metal poor dwarfs. BONIFACIO P., MOLARO P., SIVARANI T., et al.
2009ApJ...694.1577K 37           X         1 11 14 Early-age evolution of the Milky Way related by extremely metal-poor stars. KOMIYA Y., SUDA T. and FUJIMOTO M.Y.
2010A&A...515A.111S viz 15       D               1 17230 227 The PASTEL catalogue of stellar parameters. SOUBIRAN C., LE CAMPION J.-F., CAYREL DE STROBEL G., et al.
2011MNRAS.412..843S viz 76           X         2 148 109 The stellar abundances for galactic archaeology (SAGA) data base – II. Implications for mixing and nucleosynthesis in extremely metal-poor stars and chemical enrichment of the galaxy. SUDA T., YAMADA S., KATSUTA Y., et al.
2015AJ....149...39A 16       D               1 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               2 31408 141 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., 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.

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