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| HD 176465B , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST22:09:03 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2017A&A...601A..82W | 676 | X C | 16 | 13 | 29 | Kepler observations of the asteroseismic binary HD 176465. | WHITE T.R., BENOMAR O., SILVA AGUIRRE V., et al. | ||
| 2018ApJ...856..123G | 682 | X C | 16 | 6 | 3 | Asteroseismic investigations of the binary system HD 176465. | GAI N., BASU S. and TANG Y. | ||
| 2018MNRAS.477.5052N | 40 | X | 1 | 35 | 10 | Asteroseismic modelling of solar-type stars: internal systematics from input physics and surface correction methods. | NSAMBA B., CAMPANTE T.L., MONTEIRO M.J.P.F.G., et al. | ||
| 2019A&A...622A..76M | 81 | X | 2 | 30 | 3 | Seismic performance. | MOSSER B., MICHEL E., SAMADI R., et al. | ||
2021MNRAS.500...54N 
|
17 | D | 1 | 39 | 13 | Asteroseismic modelling of solar-type stars: a deeper look at the treatment of initial helium abundance. | NSAMBA B., MOEDAS N., CAMPANTE T.L., et al. | ||
|
2021AJ....162..260M
|
17 | D | 1 | 736 | ~ | Astrometric mass ratios of 248 long-period binary stars resolved in Hipparcos and Gaia EDR3. | MAKAROV V.V. and FABRICIUS C. | ||
| 2023MNRAS.522.1583K | 17 | D | 1 | 15 | 1 | Why the observed spin evolution of older-than-solar-like stars might not require a dynamo mode change. | KOTORASHVILI K., BLACKMAN E.G. and OWEN J.E. | ||
|
2023AJ....165..267H
|
17 | D | 1 | 64663 | 1 | Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O2 Levels in Nearby Transiting Habitable-zone Exoplanets. | HARDEGREE-ULLMAN K.K., APAI D., BERGSTEN G.J., et al. | ||
| 2024ApJ...962..138S | 18 | D | 1 | 56 | ~ | Stellar Cruise Control: Weakened Magnetic Braking Leads to Sustained Rapid Rotation of Old Stars. | SAUNDERS N., VAN SADERS J.L., LYTTLE A.J., et al. |
