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| V* V954 Ori , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST19:45:35 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1972IBVS..717....1K | 1829 | 16 | 58th name-list of variable stars. | KUKARKIN B.V., KHOLOPOV P.N., KUKARKINA N.P., et al. | |||||
| 1987AbaOB..62....1S | 307 | 0 | Trapezium - type multiple stellar systems in T-associations. | SALUKVADZE G.N. | |||||
| 1990BICDS..38..165S | 169 | 0 | The catalogue of multiple and double stars of T-Associations in a machine-readable form. | SALUKVADZE G.N. | |||||
|
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....157...85B |
16 | D | 1 | 2109 | 48 | The CIDA Variability Survey of Orion OB1 II. Demographics of the young, low-mass stellar populations. | BRICENO C., CALVET N., HERNANDEZ J., 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...893...56M |
16 | D | 1 | 853 | 16 | The evolution of the inner regions of protoplanetary disks. | MANZO-MARTINEZ E., CALVET N., HERNANDEZ J., et al. | ||
|
2020AJ....160..268T |
16 | D | 1 | 1158 | ~ | Statistics of wide pre-main-sequence binaries in the Orion OB1 association. | TOKOVININ A., PETR-GOTZENS M.G. and BRICENO C. | ||
|
2022AJ....163...74T |
17 | D | 3 | 191 | 7 | A census of the low accretors. I. The catalog. | THANATHIBODEE T., CALVET N., HERNANDEZ J., 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. | ||
|
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. |