HE 0015+0048 , the SIMBAD biblio

HE 0015+0048 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST22:47:35

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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
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.
2011ApJ...742...54H viz 774       D     X C       20 23 59 The Chemical Abundances of Stars in the Halo (CASH) project. II. A sample of 14 extremely metal-poor stars. HOLLEK J.K., FREBEL A., ROEDERER I.U., 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.
2016ApJ...833...20Y viz 94       D       C       3 304 147 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.
2017ApJ...835...81B viz 16       D               2 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.
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.
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.
2023MNRAS.526.4467J 235       D     X   F     5 14 ~ Rapidly rotating massive Population III stars: a solution for high carbon enrichment in CEMP-no stars. JEENA S.K., BANERJEE P., CHIAKI G., et al.

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