HE 1305+0132 , the SIMBAD biblio

HE 1305+0132 , the SIMBAD biblio (25 results) C.D.S. - SIMBAD4 rel 1.7 - 2021.01.27CET18:51:26

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Title First 3 Authors
2020ApJ...894....7Y 159       D     X C       3 16 ~ Identification of a Group III CEMP-no star in the dwarf spheroidal galaxy Canes Venatici I. YOON J., WHITTEN D.D., BEERS T.C., et al.
2020MNRAS.498.3549M 373           X C       7 15 ~ Constraining nucleosynthesis in two CEMP progenitors using fluorine. MURA-GUZMAN A., YONG D., ABATE C., et al.
2019A&A...621A.108A viz 18       D               1 59 ~ Binarity among CEMP-no stars: an indication of multiple formation pathways? ARENTSEN A., STARKENBURG E., SHETRONE M.D., et al.
2016ApJ...833...20Y viz 17       D               1 304 44 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.
2012MNRAS.419.3346G viz 16       D               1 1046 14 Revised and updated catalogue of the first byurakan survey of late-type stars. GIGOYAN K.S. and MICKAELIAN A.M.
2012MNRAS.422..849B 175       D       C F     3 97 76 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.
2011ApJ...729...40L 237           X         6 17 44 Fluorine and sodium in c-rich low-metallicity stars. LUCATELLO S., MASSERON T., JOHNSON J.A., et al.
2011MNRAS.418..284B viz 16       D               3 115 128 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.
2010ApJ...723..658O viz 195           X         5 25 35 The origin and evolution of the halo PN BoBn 1: from a viewpoint of chemical abundances based on multiwavelength spectra. OTSUKA M., TAJITSU A., HYUNG S., et al.
2010MmSAI..81..998G 79           X         2 2 7 The role of primary 16O as a neutron poison in AGB stars and fluorine primary production at halo metallicities. GALLINO R., BISTERZO S., CRISTALLO S., et al.
2010MmSAI..81.1064S 78           X         2 2 1 Mixing processes in carbon-enhanced metal-poor stars. STANCLIFFE R.J.
2009A&A...508.1359I 195           X C       4 12 67 Population synthesis of binary carbon-enhanced metal-poor stars. IZZARD R.G., GLEBBEEK E., STANCLIFFE R.J., et al.
2009ApJ...694..971A 41           X         1 7 32 Fluorine in asymptotic giant branch carbon stars revisited. ABIA C., RECIO-BLANCO A., DE LAVERNY P., et al.
2009MNRAS.394.1051S 156           X         4 9 25 Light element abundances in carbon-enhanced metal-poor stars. STANCLIFFE R.J.
2008A&A...482..151M 77               F     1 68 26 New observations of cool carbon stars in the halo. MAURON N.
2008A&A...484L..27L 759   K A     X C       19 2 26 Fluorine in carbon-enhanced metal-poor stars: a binary scenario. LUGARO M., DE MINK S.E., IZZARD R.G., et al.
2008ApJ...682L.105O 177     A     X C       4 19 23 Detection of fluorine in the halo planetary nebula BoBn 1: evidence for a binary progenitor star. OTSUKA M., IZUMIURA H., TAJITSU A., et al.
2007A&A...463..969M 51 8 The properties of carbon stars found in the Byurakan and the Hamburg/ESO surveys. MAURON N., GIGOYAN K.S. and KENDALL T.R.
2007ApJ...667L..81S 52   K     O           1 29 Fluorine in a carbon-enhanced metal-poor star. SCHULER S.C., CUNHA K., SMITH V.V., et al.
2007ApJS..168..128B viz 15       D               1851 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.
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.
2006Ap.....49..173G 47 3 Investigation of faint galactic carbon stars from the first Byurakan spectral sky survey. II. GIGOYAN K.S., MICKAELIAN A.M. and MAURON N.
2005MNRAS.359..531G 101 32 CH stars at high Galactic latitudes. GOSWAMI A.
2002Ap.....45..322G viz 161 3 First Byurakan Spectral Sky Survey types. XIII. Zone +1deg ≤ delta ≤ +13deg. GIGOYAN K.S., ABRAHAMYAN H.V., AZZOPARDI M., et al.
2001A&A...375..366C viz 410 83 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.

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