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HE 0013-0522 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.03.29CET13:48:31 |
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 |
---|---|---|---|---|---|---|---|---|---|
2006ApJ...652.1585F | 15 | D | 1775 | 155 | Bright metal-poor stars from the Hamburg/ESO survey. I. Selection and follow-up observations from 329 fields. | FREBEL A., CHRISTLIEB N., NORRIS J.E., et al. | |||
2011ApJ...742...54H | 16 | D | 5 | 23 | 59 | The Chemical Abundances of Stars in the Halo (CASH) project. II. A sample of 14 extremely metal-poor stars. | HOLLEK J.K., FREBEL A., ROEDERER I.U., et al. | ||
2014ApJ...797...21P | 16 | 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. | ||
2017ApJ...835...81B | 57 | D | X | 2 | 1801 | 18 | Bright metal-poor stars from the Hamburg/ESO Survey. II. A chemodynamical analysis. | BEERS T.C., PLACCO V.M., CAROLLO D., et al. | |
2018ApJS..239....2B | 16 | D | 1 | 4222 | 229 | A revised exoplanet yield from the Transiting Exoplanet Survey Satellite (TESS). | BARCLAY T., PEPPER J. and QUINTANA E.V. | ||
2019A&A...632A..62C | 84 | C | 1 | 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...894...34D | 17 | D | 1 | 24035 | ~ | The metallicity gradient and complex formation history of the outermost halo of the Milky Way. | DIETZ S.E., YOON J., BEERS T.C., et al. | ||
2020ApJ...898..150E | 17 | D | 1 | 144 | 41 | The r-process Alliance: first Magellan/MIKE release from the southern search for r-process-enhanced stars. | EZZEDDINE R., RASMUSSEN K., FREBEL A., et al. | ||
2021ApJ...913...11L | 17 | D | 1 | 1901 | 19 | Targeting bright metal-poor stars in the disk and halo systems of the Galaxy. | LIMBERG G., SANTUCCI R.M., ROSSI S., et al. |