HE 1052-2548 , the SIMBAD biblio

HE 1052-2548 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST22:48:28


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Title First 3 Authors
2005A&A...439..129B viz 15       D               1 252 422 The Hamburg/ESO R-process enhanced star survey (HERES). II. Spectroscopic analysis of the survey sample. BARKLEM P.S., CHRISTLIEB N., BEERS T.C., et al.
2006ApJ...652.1585F viz 15       D               1775 155 Bright metal-poor stars from the Hamburg/ESO survey. I. Selection and follow-up observations from 329 fields. FREBEL A., CHRISTLIEB N., NORRIS J.E., et al.
2007ApJS..168..128B viz 15       D               1852 38 Broadband UBVRCIC photometry of horizontal-branch and metal-poor candidates from the HK and Hamburg/ESO surveys. I. BEERS T.C., FLYNN C., ROSSI S., et al.
2009AJ....137..272R viz 15       D               1 737 45 Chemical inhomogeneities in the Milky Way stellar halo. ROEDERER I.U.
2011A&A...528A..92Z viz 15       D               1 254 10 The Hamburg/ESO R-process Enhanced Star survey (HERES). VI. The Galactic chemical evolution of silicon. ZHANG L., KARLSSON T., CHRISTLIEB N., et al.
2012A&A...537A.118R 15       D               1 112 9 The Hamburg/ESO R-process Enhanced Star survey (HERES). VII. Thorium abundances in metal-poor stars. REN J., CHRISTLIEB N. and ZHAO G.
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.
2017ApJ...835...81B viz 16       D               1 1801 18 Bright metal-poor stars from the Hamburg/ESO Survey. II. A chemodynamical analysis. BEERS T.C., PLACCO V.M., CAROLLO D., et al.
2022ApJ...940..159P 18       D               2 37 2 Very Metal-poor Stars in the Solar Vicinity: Age Determination. PLOTNIKOVA A., CARRARO G., VILLANOVA S., et al.
2023ApJ...949...31P 19       D               1 33 1 Very Metal-poor Stars in the Solar Vicinity: Kinematics and Abundance Analysis. PLOTNIKOVA A., CARRARO G., VILLANOVA S., et al.

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