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| TYC 7629-1640-1 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST05:17:15 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 1979ApJ...230..786E | 324 | 28 | Luminosity and motion of large proper-motion stars. I. Stars with annual proper motion larger than 1". | EGGEN O.J. | |||||
| 1979ApJS...39...89E | 410 | 89 | Catalogs of proper-motion stars. I. Stars brighter than visual magnitude 15 and with annual proper motion of 1" or more. | EGGEN O.J. | |||||
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. | ||
|
2018A&A...620A.172Z
|
16 | D | 1 | 127610 | 99 | 3D mapping of young stars in the solar neighbourhood with Gaia DR2. | ZARI E., HASHEMI H., BROWN A.G.A., 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. | ||
|
2021MNRAS.503.3279S
|
17 | D | 1 | 104620 | 56 | The GALAH survey: tracing the Galactic disc with open clusters. | SPINA L., TING Y.-S., DE SILVA G.M., et al. | ||
|
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. | ||
|
2022ApJS..262....7H
|
17 | D | 1 | 134735 | 19 | A Blind All-sky Search for Star Clusters in Gaia EDR3: 886 Clusters within 1.2 kpc of the Sun. | HE Z., WANG K., LUO Y., et al. | ||
|
2023A&A...678A..75Z
|
17 | D | 1 | 27445 | ~ | Young nearby open clusters and their luminosity functions. | ZERJAL M., LODIEU N., PEREZ-GARRIDO A., 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. |
