|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| TYC 4765-319-1 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST11:39:50 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
1954TrSht..25....1P |
2988 | 88 | Catalogue of stars in the area of the Orion Nebula. | PARENAGO P.P. | |||||
|
1992BICDS..40...13M |
2986 | 2 | Machine-readable version of the Parenago catalogue of stars in the area of the Orion nebula. | MALKOV O.Y. | |||||
|
2018MNRAS.475.5659W |
16 | D | 1 | 3232 | 30 | Not all stars form in clusters - measuring the kinematics of OB associations with Gaia. | WARD J.L. and KRUIJSSEN J.M.D. | ||
|
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. | ||
|
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...931..156P |
17 | D | 1 | 22106 | 16 | 3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR 3. II. Hierarchical Star Formation Revealed by Spatial and Kinematic Substructures. | PANG X., TANG S.-Y., LI Y., et al. | ||
|
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. | ||
|
2023AJ....166..189R |
87 | C | 1 | 21 | ~ | Machine-learning Morphological Classification of TESS Light Curves of T Tauri Stars. | RODRIGUEZ-FELICIANO B., SERNA J., GARCIA-VARELA 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. |