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| Haro 4-117 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST09:16:14 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1953ApJ...117...73H | 270 | 119 | H-alpha emission stars and peculiar objects in the region of the Orion Nebula. | HARO G. | |||||
|
1982BITon...3...69P |
14 | D | 1 | 541 | 46 | Catalog of H-alpha emission stars in the region of the Orion nebula. | PARSAMIAN E.S. and CHAVIRA E. | ||
|
2000AJ....119.3026R |
1850 | 55 | Circumstellar disk candidates identified from ultraviolet excesses in the Orion nebula cluster flanking fields. | REBULL L.M., HILLENBRAND L.A., STROM S.E., et al. | |||||
|
2008ApJ...676.1109F |
15 | D | 1 | 1217 | 126 | Kinematic structure of the Orion Nebula Cluster and its surroundings. | FURESZ G., HARTMANN L.W., MEGEATH S.T., et al. | ||
|
2009ApJ...697.1103T |
15 | D | 1 | 1591 | 133 | Kinematics of the Orion Nebula Cluster: velocity substructure and spectroscopic binaries. | TOBIN J.J., HARTMANN L., FURESZ G., et al. | ||
|
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. | ||
|
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. | ||
|
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. |