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| HE 0405-0526 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST16:31:33 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2016A&A...586A.160H | 449 | D | O X C | 11 | 36 | 87 | The role of binaries in the enrichment of the early Galactic halo. II. Carbon-enhanced metal-poor stars: CEMP-no stars. | HANSEN T.T., ANDERSEN J., NORDSTROEM B., et al. | |
|
2016ApJ...833...20Y |
16 | D | 2 | 304 | 147 | 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. | ||
|
2018AJ....156...18P |
16 | D | 1 | 51824 | 872 | Binary companions of evolved stars in APOGEE DR14: search method and catalog of ∼5000 companions. | PRICE-WHELAN A.M., HOGG D.W., RIX H.-W., et al. | ||
|
2019A&A...621A.108A |
16 | D | 2 | 59 | 49 | Binarity among CEMP-no stars: an indication of multiple formation pathways? | ARENTSEN A., STARKENBURG E., SHETRONE M.D., et al. | ||
| 2019ApJ...879...37N | 16 | D | 1 | 74 | 7 | The most metal-poor stars. V. The CEMP-no stars in 3D and non-LTE. | NORRIS J.E. and YONG D. | ||
|
2020AJ....160..120J |
16 | D | 1 | 365763 | 238 | APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. | JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al. | ||
|
2022AJ....163..152S |
17 | D | 1 | 583193 | 11 | APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. | SPRAGUE D., CULHANE C., KOUNKEL M., et al. | ||
|
2022ApJS..259...35A |
17 | D | 1 | 611005 | 320 | The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. | ABDURRO'UF, ACCETTA K., AERTS C., et al. | ||
|
2023ApJ...947...23Z |
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. |