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| V* V1173 Ori , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST07:09:14 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1979IBVS.1628....1C | 11 | 3 | Flare stars in Orion. | CHAVUSHIAN H.S., MELIKIAN N.D., MIRZOYAN L.V., et al. | |||||
| 1987ATsir1476....1V | 106 | 0 | An analysis of the Large Telescope Optics. | VITRICHENKO E.A. and PUSCHNOY L.A. | |||||
|
1987IBVS.3058....1K |
667 | 121 | The 68th name-list of variable stars. | KHOLOPOV P.N., SAMUS' N.N., KAZAROVETS E.V., et al. | |||||
|
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. | ||
|
2014A&A...570A..30P |
15 | D | 1 | 1688 | 4 | Hα emission-line stars in molecular clouds. II. The M 42 region. | PETTERSSON B., ARMOND T. and REIPURTH B. | ||
|
2016ApJ...821....8K |
16 | D | 1 | 1943 | 23 | Spectroscopic binaries in the Orion nebula cluster and NGC 2264. | KOUNKEL M., HARTMANN L., TOBIN J.J., et al. | ||
|
2017AJ....153..188F |
16 | D | 1 | 810 | 40 | NGC 1980 is not a foreground population of Orion: spectroscopic survey of young stars with low extinction in Orion A. | FANG M., KIM J.S., PASCUCCI I., et al. | ||
|
2019ApJ...884....6M |
16 | D | 1 | 5695 | 27 | Runaway young stars near the Orion Nebula. | McBRIDE A. and KOUNKEL M. | ||
|
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. |