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| NSV 1302 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST13:46:57 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1975IBVS.1008....1G | 9 | 0 | New variable stars in a field around 38 omicron Per. | GIESEKING F. | |||||
|
2004yCat.2250....0S |
3358 | 107 | Combined General Catalogue of Variable Stars. | SAMUS N.N. and DURLEVICH O.V. | |||||
|
2015AJ....150...95A |
16 | D | 1 | 239 | 8 | A WISE census of young stellar objects in the Perseus OB2 association. | AZIMLU M., MARTINEZ-GALARZA J.R. and MUENCH A.A. | ||
|
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.503.3232P |
17 | D | 1 | 923 | 15 | The substructure of the Perseus star-forming region: a survey with Gaia DR2. | PAVLIDOU T., SCHOLZ A. and TEIXEIRA P.S. | ||
|
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. | ||
|
2022AJ....164...57K |
17 | D | 1 | 844 | 7 | Dynamical Star-forming History of Per OB2. | KOUNKEL M., DENG T. and STASSUN K.G. | ||
|
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. | ||
|
2023ApJS..265...12Q |
17 | D | 1 | 58898 | 5 | Hunting for Neighboring Open Clusters with Gaia DR3: 101 New Open Clusters within 500 pc. | QIN S., ZHONG J., TANG T., 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. |