|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| HD 221157B , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST07:30:59 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1993A&AS...98...17S | 115 | 2 | A photometric study of wide visual double stars. IV. uvby photometry of wide visual double stars with G-type primaries. | SINACHOPOULOS D. and VAN DESSEL E. | |||||
|
2017AJ....153..257O |
16 | D | 1 | 10625 | 142 | Comoving stars in Gaia DR1: an abundance of very wide separation comoving pairs. | OH S., PRICE-WHELAN A.M., HOGG D.W., et al. | ||
|
2017MNRAS.472..675A |
16 | D | 1 | 13582 | 89 | Wide binaries in Tycho-Gaia: search method and the distribution of orbital separations. | ANDREWS J.J., CHANAME J. and AGUEROS M.A. | ||
|
2018A&A...609A.116R |
16 | D | 1 | 143018 | 65 | Empirical photometric calibration of the Gaia red clump: Colours, effective temperature, and absolute magnitude. | RUIZ-DERN L., BABUSIAUX C., ARENOU F., et al. | ||
|
2018AJ....155..149B |
16 | D | 1 | 9764 | 5 | Fundamental properties of co-moving stars observed by Gaia. | BOCHANSKI J.J., FAHERTY J.K., GAGNE J., et al. | ||
|
2021ApJ...921..118N |
17 | D | 2 | 70 | 14 | Distant relatives: the chemical homogeneity of comoving pairs identified in Gaia. | NELSON T., TING Y.-S., HAWKINS K., et al. | ||
|
2022MNRAS.514.1071M |
17 | D | 1 | 2315 | ~ | A measurement of stellar surface gravity hidden in radial velocity differences of comoving stars. | MOSCHELLA M., SLONE O., DROR J.A., et al. | ||
|
2024Natur.627..501L |
18 | D | 1 | 246 | ~ | At least one in a dozen stars shows evidence of planetary ingestion. | LIU F., TING Y.-S., YONG D., et al. | ||
| 2025MNRAS.538.2408Y | 93 | F | 1 | 11 | ~ | C3PO - IV. Co-natal stars depleted in refractories are magnetically more active - possible imprints of planets. | YU J., TING Y.-S., CASAGRANDE L., et al. |