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HE 0044-2459 , the SIMBAD biblio (22 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST12:25:38 |
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 |
---|---|---|---|---|---|---|---|---|---|
1985AJ.....90.2089B | 167 | 348 | A search for stars of very low metal abundance. I. | BEERS T.C., PRESTON G.W. and SHECTMAN S.A. | |||||
1986ApJS...61..667N | 937 | 212 | Population studies. II. Kinematics as a function of abundance and galactocentric position for Fe/H -0.6. | NORRIS J. | |||||
1991ApJS...76.1001P | 1762 | 52 | Photoelectric UBV photometry of stars selected in the HK objective-prism survey. | PRESTON G.W., SHECTMAN S.A. and BEERS T.C. | |||||
1992AJ....103.1987B | 1024 | 532 | A search for stars of very low metal abundance. II. | BEERS T.C., PRESTON G.W. and SHECTMAN S.A. | |||||
1995ApJS...96..175B | 1810 | 175 | Kinematics of metal-poor stars in the Galaxy. | BEERS T.C. and SOMMER-LARSEN J. | |||||
1999ApJS..123..639N | 2628 | 37 | A search for stars of very low metal abundance. III. UBV photometry of metal-weak candidates. | NORRIS J.E., RYAN S.G. and BEERS T.C. | |||||
2000AJ....119.2866B | 2011 | 171 | Kinematics of metal-poor stars in the Galaxy. II. Proper motions for a large nonkinematically selected sample. | BEERS T.C., CHIBA M., YOSHII Y., et al. | |||||
2004AJ....128.2402L | 135 | 16 | Abundances of extremely metal-poor star candidates. | LAI D.K., BOLTE M., JOHNSON J.A., et al. | |||||
2005A&A...439..129B | 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 | 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. | |||
2009AJ....137..272R | 15 | D | 1 | 737 | 45 | Chemical inhomogeneities in the Milky Way stellar halo. | ROEDERER I.U. | ||
2011A&A...528A..92Z | 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. | ||
2014AJ....147..136R | 16 | D | 4 | 317 | 336 | A search for stars of very low metal abundance. VI. Detailed abundances of 313 metal-poor stars. | ROEDERER I.U., PRESTON G.W., THOMPSON I.B., et al. | ||
2014ApJ...797...21P | 16 | D | 4 | 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. | ||
2016A&A...591A.118S | 16 | D | 1 | 31406 | 141 | The PASTEL catalogue: 2016 version. | SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al. | ||
2018ApJ...857...46I | 16 | D | 1 | 205 | 88 | The initial mass function of the first stars inferred from extremely metal-poor stars. | ISHIGAKI M.N., TOMINAGA N., KOBAYASHI C., et al. | ||
2018ApJ...857..111T | 17 | D | 1 | 73 | 76 | Stellar yields of rotating first stars. II. Pair-instability supernovae and comparison with observations. | TAKAHASHI K., YOSHIDA T. and UMEDA H. | ||
2019A&A...632A..62C | 84 | C | 3 | 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...900..106O | 17 | D | 1 | 314 | ~ | Vanadium abundance derivations in 255 metal-poor stars. | OU X., ROEDERER I.U., SNEDEN C., et al. | ||
2021ApJ...907...10L | 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. | ||
2022A&A...661A.153M | 18 | D | 3 | 58 | 4 | Discovery of a thin lithium plateau among metal-poor red giant branch stars,. | MUCCIARELLI A., MONACO L., BONIFACIO P., et al. | ||
2024ApJS..270...28R | 20 | D | 1 | 54 | ~ | Zero and Extremely Low-metallicity Rotating Massive Stars: Evolution, Explosion, and Nucleosynthesis Up to the Heaviest Nuclei. | ROBERTI L., LIMONGI M. and CHIEFFI A. |