HE 0400-2030 , the SIMBAD biblio

HE 0400-2030 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST17:54:57

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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
2001A&A...375..366C viz 410 121 The stellar content of the Hamburg/ESO survey. II. A large, homogeneously-selected sample of high latitude carbon stars. CHRISTLIEB N., GREEN P.J., WISOTZKI L., 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.
2007ApJ...655..492A viz 2 70 376 Carbon-enhanced metal-poor stars. I. Chemical compositions of 26 stars. AOKI W., BEERS T.C., CHRISTLIEB N., et al.
2007BASI...35..339G 68 7 Low-resolution spectroscopy of high galactic latitude objects: A search for CH stars. GOSWAMI A., BAMA P., SHANTIKUMAR N.S., et al.
2009MNRAS.396.1046L 40           X         1 7 35 The evolution of low-metallicity asymptotic giant branch stars and the formation of carbon-enhanced metal-poor stars. LAU H.H.B., STANCLIFFE R.J. and TOUT C.A.
2009A&A...508.1359I 43           X         1 12 141 Population synthesis of binary carbon-enhanced metal-poor stars. IZZARD R.G., GLEBBEEK E., STANCLIFFE R.J., et al.
2010A&A...509A..93M viz 15       D               2 181 196 A holistic approach to carbon-enhanced metal-poor stars. MASSERON T., JOHNSON J.A., PLEZ B., et al.
2011MNRAS.412..843S viz 131       D     X         4 148 109 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.
2011MNRAS.418..284B viz 15       D               3 115 191 The s-process in low-metallicity stars – II. Interpretation of high-resolution spectroscopic observations with asymptotic giant branch models. BISTERZO S., GALLINO R., STRANIERO O., et al.
2012MNRAS.422..849B 93       D         F     2 97 85 The s-process in low-metallicity stars - III. Individual analysis of CEMP-s and CEMP-s/r with asymptotic giant branch models. BISTERZO S., GALLINO R., STRANIERO O., et al.
2012A&A...547A..76P 93       D   O X         3 19 25 The occurrence of nitrogen-enhanced metal-poor stars: implications for the initial mass function in the early Galactic halo. POLS O.R., IZZARD R.G., STANCLIFFE R.J., et al.
2013ApJ...762...26Y viz 16       D               1 198 263 The most metal-poor stars. II. Chemical abundances of 190 metal-poor stars including 10 new stars with [Fe/H] ≤ -3.5. YONG D., NORRIS J.E., BESSELL M.S., et al.
2012A&A...548A..34A viz 15       D               4 134 38 Elemental abundances and classification of carbon-enhanced metal-poor stars. ALLEN D.M., RYAN S.G., ROSSI S., et al.
2014ApJ...788..180C viz 16       D               1 329 52 Carbon-enhanced metal-poor stars: CEMP-s and CEMP-no subclasses in the halo system of the Milky Way. CAROLLO D., FREEMAN K., BEERS T.C., et al.
2016A&A...588A..37H 417       D   O X C       10 33 24 Abundances of carbon-enhanced metal-poor stars as constraints on their formation. HANSEN C.J., NORDSTROM B., HANSEN T.T., et al.
2016ApJ...833...20Y viz 16       D               1 304 147 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.
2019A&A...623A.128H viz 17       D               1 100 36 Abundances and kinematics of carbon-enhanced metal-poor stars in the Galactic halo. A new classification scheme based on Sr and Ba. HANSEN C.J., HANSEN T.T., KOCH A., et al.
2020A&A...634A..72S 17       D               4 83 ~ An empirical metallicity tracer in CEMP and C-normal stars. SINGH D., HANSEN C.J., BYRGESEN J.S., 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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