HE 1219-0312 , the SIMBAD biblio

HE 1219-0312 , the SIMBAD biblio (50 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST03:51:22

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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
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.
2006A&A...451..651J 1 44 134 The Hamburg/ESO R-process enhanced star survey (HERES). III. HE 0338-3945 and the formation of the r + s stars. JONSELL K., BARKLEM P.S., GUSTAFSSON B., 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.
2009ApJ...698.1963R 427       D     X C F     10 57 66 The end of nucleosynthesis: production of lead and thorium in the early galaxy. ROEDERER I.U., KRATZ K.-L., FREBEL A., et al.
2009A&A...504..511H 3184 T   A D   O X C       84 10 33 The Hamburg/ESO R-process enhanced star survey (HERES). IV. Detailed abundance analysis and age dating of the strongly r-process enhanced stars CS 29491-069 and He
1219-0312. 		HAYEK W., WIESENDAHL U., CHRISTLIEB N., 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.
2010A&A...516A..46M viz 288     A     X C       7 9 42 The Hamburg/ESO R-process enhanced star survey (HERES). V. Detailed abundance analysis of the r-process enhanced star HE 2327-5642. MASHONKINA L., CHRISTLIEB N., BARKLEM P.S., et al.
2010ApJ...724..975R viz 90       D       C       2 197 141 The ubiquity of the rapid neutron-capture process. ROEDERER I.U., COWAN J.J., KARAKAS A.I., et al.
2010MNRAS.409.1068Z 90       D         F     2 14 8 A holistic abundance analysis of r-rich stars. ZHANG J., CUI W. and ZHANG B.
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.
2011AstL...37..480S 13 4 The r- and s-process contributions to heavy-element abundances in the halo star HD 29907. SITNOVA T.M. and MASHONKINA L.I.
2011A&A...534A..60B 38           X         1 11 20 First stars. XV. Third-peak r-process element and actinide abundances in the uranium-rich star CS 31082-001. BARBUY B., SPITE M., HILL V., et al.
2011ApJ...743L...1H 15       D               1 19 26 The binary frequency of r-process-element-enhanced metal-poor stars and its implications: chemical tagging in the primitive halo of the Milky way. HANSEN T., ANDERSEN J., NORDSTROM B., et al.
2011MNRAS.418..284B viz 114           X C       2 115 191 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.
2012A&A...537A.118R 130       D     X         4 112 9 The Hamburg/ESO R-process Enhanced Star survey (HERES). VII. Thorium abundances in metal-poor stars. REN J., CHRISTLIEB N. and ZHAO G.
2012A&A...545A..31H 15       D               2 74 111 Silver and palladium help unveil the nature of a second r-process. HANSEN C.J., PRIMAS F., HARTMAN H., et al.
2013PASP..125..143L 207       D     X C       5 31 11 Study of neutron-capture element abundances in metal-poor stars. LI H., SHEN X., LIANG S., et al.
2013A&A...551A..57H 15       D   O           2 73 63 LTE or non-LTE, that is the question. The NLTE chemical evolution of strontium in extremely metal-poor stars. HANSEN C.J., BERGEMANN M., CESCUTTI G., et al.
2013A&A...558A..36C 38           X         1 21 13 The Hamburg/ESO R-process Enhanced Star survey (HERES). VIII. The r+s star He 1405-0822. CUI W.Y., SIVARANI T. and CHRISTLIEB N.
2014A&A...565A.123M 325       D     X C       8 19 8 The Hamburg/ESO R-process Enhanced Star survey (HERES). IX. Constraining pure r-process Ba/Eu abundance ratio from observations of r-II stars. MASHONKINA L. and CHRISTLIEB N.
2014A&A...568A..47H 15       D               1 72 16 Stellar abundances and presolar grains trace the nucleosynthetic origin of molybdenum and ruthenium. HANSEN C.J., ANDERSEN A.C. and CHRISTLIEB N.
2014A&A...569A..43M viz 255     A     X C       6 14 26 The Hamburg/ESO R-process Enhanced Star survey (HERES). X. HE 2252-4225, one more r-process enhanced and actinide-boost halo star. MASHONKINA L., CHRISTLIEB N. and ERIKSSON K.
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.
2015ApJ...813...56N 78           X         2 12 3 Study of the element abundances in HD 140283: the abundance robustness of the weak r- and main r-process stars. NIU P., CUI W. and ZHANG B.
2015A&A...583A..49H 211       D   O X C       5 31 28 The role of binaries in the enrichment of the early Galactic halo. I. r-process-enhanced metal-poor stars. HANSEN T.T., ANDERSEN J., NORDSTROEM B., et al.
2015A&A...583A..67J 235           X C       5 21 43 The early days of the Sculptor dwarf spheroidal galaxy. JABLONKA P., NORTH P., MASHONKINA L., et al.
2017ApJ...844...18P viz 41           X         1 8 23 RAVE J203843.2-002333: the first highly r-process-enhanced star identified in the RAVE survey. PLACCO V.M., HOLMBECK E.M., FREBEL A., et al.
2017A&A...608A..89M viz 40           X         1 75 50 The formation of the Milky Way halo and its dwarf satellites: a NLTE-1D abundance analysis. II. Early chemical enrichment. MASHONKINA L., JABLONKA P., SITNOVA T., et al.
2018ApJ...854..131W 1485     A D     X C       37 9 ~ The odd isotope fractions of barium in the strongly r-process-enhanced (r-II) stars. WENYUAN C., XIAOHUA J., JIANRONG S., et al.
2018AJ....156..179R viz 16       D               1 90 63 Kinematics of highly r-process-enhanced field stars: evidence for an accretion origin and detection of several groups from disrupted satellites. ROEDERER I.U., HATTORI K. and VALLURI M.
2019ApJ...882...40J viz 16       D               2 210 41 The lanthanide fraction distribution in metal-poor stars: a test of neutron star mergers as the dominant r-process site. JI A.P., DROUT M.R. and HANSEN T.T.
2020A&A...634A..72S 16       D               1 83 ~ An empirical metallicity tracer in CEMP and C-normal stars. SINGH D., HANSEN C.J., BYRGESEN J.S., et al.
2020ApJ...900..179K 99             C       1 17 289 The origin of elements from carbon to uranium. KOBAYASHI C., KARAKAS A.I. and LUGARO M.
2021ApJ...909...21H 17       D               1 33 11 Reconstructing masses of merging neutron stars from stellar r-process abundance signatures. HOLMBECK E.M., FREBEL A., McLAUGHLIN G.C., et al.
2022A&A...661A.153M viz 17       D               4 58 4 Discovery of a thin lithium plateau among metal-poor red giant branch stars,. MUCCIARELLI A., MONACO L., BONIFACIO P., et al.
2022A&A...663A..70F 17       D               1 47 17 Correlations of r-process elements in very metal-poor stars as clues to their nucleosynthesis sites. FAROUQI K., THIELEMANN F.-K., ROSSWOG S., et al.
2022ApJ...936...84R 43           X         1 21 7 The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks. ROEDERER I.U., COWAN J.J., PIGNATARI M., et al.
2022A&A...665A..10L viz 17       D               1 56 8 Chemical Evolution of R-process Elements in Stars (CERES). I. Stellar parameters and chemical abundances from Na to Zr. LOMBARDO L., BONIFACIO P., FRANCOIS P., et al.
2023ApJ...943...23S viz 17       D               1 1792 5 The R-Process Alliance: Chemodynamically Tagged Groups. II. An Extended Sample of Halo r-process-enhanced Stars. SHANK D., BEERS T.C., PLACCO V.M., et al.
2023ApJ...946...48H viz 17       D               2 181 5 Finding r-II Sibling Stars in the Milky Way with the Greedy Optimistic Clustering Algorithm. HATTORI K., OKUNO A. and ROEDERER I.U.
2023ApJ...959...60P 17       D               1 38 ~ SPLUS J142445.34-254247.1: An r-process-enhanced, Actinide-boost, Extremely Metal-poor Star Observed with GHOST. PLACCO V.M., ALMEIDA-FERNANDES F., HOLMBECK E.M., et al.
2024ApJ...970L..30X 18       D               1 81 ~ Discovery of an Extremely r-process-enhanced Thin-disk Star with [Eu/H] = +0.78. XIE X.-J., SHI J., YAN H.-L., et al.
2024ApJ...971..158R 18       D               1 48 ~ The R-Process Alliance: 2MASS J22132050-5137385, the Star with the Highest-known r-process Enhancement at [Eu/Fe] = +2.45. ROEDERER I.U., BEERS T.C., HATTORI K., et al.
2024A&A...691A.220F 18       D               3 54 ~ Chemical Evolution of R-process Elements in Stars (CERES) II. The impact of stellar evolution and rotation on light and heavy elements. FERNANDES DE MELO R., LOMBARDO L., ALENCASTRO PULS A., et al.
2024A&A...691A.284R viz 18       D               1 80 ~ The earliest phases of CNO enrichment in galaxies. ROSSI M., ROMANO D., MUCCIARELLI A., et al.
2025A&A...693A.293L viz 252       D     X C       5 32 ~ Chemical Evolution of R-process Elements in Stars (CERES) III. Chemical abundances of neutron capture elements from Ba to Eu. LOMBARDO L., HANSEN C.J., RIZZUTI F., et al.
2025A&A...693A.294A 19       D               1 58 ~ Chemical Evolution of R-process Elements in Stars (CERES) IV. An observational run-up of the third r-process peak with Hf, Os, Ir, and Pt. ALENCASTRO PULS A., KUSKE J., HANSEN C.J., et al.
2025ApJ...992...56T 93           X         2 13 ~ Study of Neutron Capture Nucleosynthesis Based on Post-Asymptotic Giant Branch Stars. TIAN M., CUI W., SHI J.-R., et al.
2025ApJ...992...36V 19       D               1 42 ~ Classifying Metal-poor Stars with Machine Learning Using Nucleosynthesis Calculations. VASSH N., WANG Y., WOLOSHYN R.M., et al.
2025A&A...703A.296M 345       D     X C       7 48 ~ Understanding the origin of palladium in metal-poor stars based on the non-local thermodynamic equilibrium analysis of Pd I lines. MASHONKINA L. and SMOGORZHEVSKII A.

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