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| TYC 9210-1484-1 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST03:44:36 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2016MNRAS.461..794P |
16 | D | 1 | 802 | 260 | The star formation history and accretion-disc fraction among the K-type members of the Scorpius-Centaurus OB association. | PECAUT M.J. and MAMAJEK E.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. | ||
|
2017A&A...601A..19G |
16 | D | 1 | 1218 | 88 | Gaia Data Release 1. Open cluster astrometry: performance, limitations, and future prospects. | GAIA COLLABORATION, VAN LEEUWEN F., VALLENARI A., 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...616A..10G |
16 | D | 1 | 40955 | 656 | Gaia Data Release 2. Observational Hertzsprung-Russell diagrams. | GAIA COLLABORATION, BABUSIAUX C., VAN LEEUWEN F., 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. | ||
|
2020ApJ...890...46T |
16 | D | 1 | 403 | 45 | Superflares on solar-type stars from the first year observation of TESS. | TU Z.-L., YANG M., ZHANG Z.J., et al. | ||
|
2021A&A...645A..84M |
17 | D | 1 | 7942 | 60 | Extended stellar systems in the solar neighborhood. V. Discovery of coronae of nearby star clusters. | MEINGAST S., ALVES J. and ROTTENSTEINER A. | ||
|
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. |