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| TYC 8273-917-1 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST22:00:49 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
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. | ||
|
2018ApJ...860...43G
|
16 | D | 2 | 739 | 55 | BANYAN. XII. New members of nearby young associations from Gaia-Tycho data. | GAGNE J., ROY-LOUBIER O., FAHERTY J.K., et al. | ||
|
2018ApJ...868...32G
|
16 | D | 1 | 1859 | 7 | A large moving group within the Lower Centaurus Crux association. | GOLDMAN B., ROSER S., SCHILBACH E., et al. | ||
|
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. | ||
|
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. | ||
|
2022AJ....164..213G
|
17 | D | 1 | 124 | 2 | Correcting Stellar Flare Frequency Distributions Detected by TESS and Kepler. | GAO D.-Y., LIU H.-G., YANG M., et al. | ||
|
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. | ||
|
2023A&A...677A..59R
|
17 | D | 1 | 13197 | ~ | Significance mode analysis (SigMA) for hierarchical structures An application to the Sco-Cen OB association. | RATZENBOCK S., GROSSSCHEDL J.E., MOLLER T., 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. |
