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| TYC 4046-788-1 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST14:25:50 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
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. | ||
|
2018A&A...615A..49C |
16 | D | 1 | 224763 | 54 | Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution. | CANTAT-GAUDIN T., VALLENARI A., SORDO R., et al. | ||
| 2018ApJ...863...91F | 16 | D | 1 | 289 | 47 | New and known moving groups and clusters identified in a Gaia comoving catalog. | FAHERTY J.K., BOCHANSKI J.J., GAGNE J., et al. | ||
|
2019AJ....158..122K |
16 | D | 1 | 290057 | 150 | Untangling the Galaxy. I. Local structure and star formation history of the Milky Way. | KOUNKEL M. and COVEY K. | ||
|
2022ApJ...928...70C |
17 | D | 1 | 5007 | 6 | Pearls on a String: Numerous Stellar Clusters Strung Along the Same Orbit. | CORONADO J., FURNKRANZ V. and RIX H.-W. | ||
|
2022ApJ...939...94M |
17 | D | 1 | 6091 | 6 | New Coronae and Stellar Associations Revealed by a Clustering Analysis of the Solar Neighborhood. | MORANTA L., GAGNE J., COUTURE D., et al. | ||
|
2024AJ....167..210V |
18 | D | 1 | 7289 | ~ | The Occurrence of Small, Short-period Planets Younger than 200 Myr with TESS. | VACH S., ZHOU G., HUANG C.X., et al. |