HE 0305-4520 , the SIMBAD biblio

HE 0305-4520 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST22:39:37


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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.
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.
2008ApJ...687..272Q 112           X C       2 29 57 Abundances of Sr, Y, and Zr in metal-poor stars and implications for chemical evolution in the early galaxy. QIAN Y.-Z. and WASSERBURG G.J.
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.
2013ApJ...766L..13A 116           X         3 11 24 Explaining the Sr and Ba scatter in extremely metal-poor stars. AOKI W., SUDA T., BOYD R.N., et al.
2014A&A...571A..40S viz 464     A D     X C       12 12 8 The low Sr/Ba ratio on some extremely metal-poor stars. SPITE M., SPITE F., BONIFACIO P., 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...830...61F 79             C       1 9 ~ Dependence of the Sr-to-Ba and Sr-to-Eu ratio on the nuclear equation of state in metal-poor halo stars. FAMIANO M.A., KAJINO T., AOKI W., et al.
2020A&A...640A..87M 100       D     X         3 23 29 Facing problems in the determination of stellar temperatures and gravities: Galactic globular clusters. MUCCIARELLI A. and BONIFACIO P.
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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