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| 2MASS J05354871-0542143 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST19:26:45 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
1995AJ....109..709A |
1723 | 62 | A 2.2 mu.m imaging survey of the Orion A molecular cloud. | ALI B. and DEPOY D.L. | |||||
|
2009ApJS..183..261D |
15 | D | 2 | 2645 | 47 | A multi-color optical survey of the Orion nebula cluster. I. The catalog. | DA RIO N., ROBBERTO M., SODERBLOM D.R., et al. | ||
|
2010ApJ...722.1092D |
15 | D | 1 | 1021 | 140 | A multi-color optical survey of the Orion Nebula Cluster. II. The H-R diagram. | DA RIO N., ROBBERTO M., SODERBLOM D.R., et al. | ||
|
2012ApJ...748...14D |
15 | D | 1 | 1754 | 122 | The initial mass function of the Orion Nebula Cluster across the H-burning limit. | DA RIO N., ROBBERTO M., HILLENBRAND L.A., et al. | ||
|
2012ApJ...755..154M |
15 | D | 1 | 715 | 76 | Hubble Space Telescope measures of mass accretion rates in the Orion Nebula Cluster. | MANARA C.F., ROBBERTO M., DA RIO N., et al. | ||
|
2019MNRAS.487.2977G |
16 | D | 1 | 1517 | 33 | Gaia stellar kinematics in the head of the Orion A cloud: runaway stellar groups and gravitational infall. | GETMAN K.V., FEIGELSON E.D., KUHN M.A., et al. | ||
|
2019ApJ...884....6M |
16 | D | 1 | 5695 | 27 | Runaway young stars near the Orion Nebula. | McBRIDE A. and KOUNKEL M. | ||
|
2021MNRAS.503.3279S |
17 | D | 1 | 104620 | 56 | The GALAH survey: tracing the Galactic disc with open clusters. | SPINA L., TING Y.-S., DE SILVA G.M., et al. | ||
|
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. |