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| UCAC4 151-113752 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST16:47:55 |
Sort references on where and how often the object is cited
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 |
|---|---|---|---|---|---|---|---|---|---|
| 1996AJ....112..693P | 8 | 8 | A new stellar nursery in the Southern Cross. | PARK S. and FINLEY J.P. | |||||
| 2002A&A...384..521A | 22 | 12 | Characterization of low-mass pre-main sequence stars in the Southern Cross. | ALCALA J.M., COVINO E., MELO C., et al. | |||||
2018ApJ...862..138G 
|
16 | D | 1 | 943 | 100 | BANYAN. XIII. A first look at nearby young associations with Gaia Data Release 2. | GAGNE J. and FAHERTY J.K. | ||
|
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. | ||
|
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. | ||
|
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. | ||
|
2023A&A...674A..21M
|
17 | D | 1 | 11510 | 8 | Gaia Data Release 3 Validating the classification of variable young stellar object candidates. | MARTON G., ABRAHAM P., RIMOLDINI L., 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. |
