[HR92] 33 , the SIMBAD biblio

[HR92] 33 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST17:30:41


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Title First 3 Authors
1992AJ....104.2193H 63 79 Kinematics and evolution of the HH 34 complex. HEATHCOTE S. and REIPURTH B.
2008ApJ...676.1109F viz 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 viz 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.
2009A&A...504..461F viz 15       D               2 439 209 Star and protoplanetary disk properties in Orion's suburbs. FANG M., VAN BOEKEL R., WANG W., et al.
2012ApJ...752...59H viz 15       D               1 987 40 The low-mass stellar population in L1641: evidence for environmental dependence of the stellar initial mass function. HSU W.-H., HARTMANN L., ALLEN L., et al.
2013ApJ...768...99P viz 16       D               1 996 33 An X-ray survey of the young stellar population of the Lynds 1641 and iota Orionis regions. PILLITTERI I., WOLK S.J., MEGEATH S.T., et al.
2013ApJS..207....5F viz 16       D               1 1421 96 Young stellar objects in Lynds 1641: disks, accretion, and star formation history. FANG M., KIM J.S., VAN BOEKEL R., et al.
2016ApJ...821....8K viz 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 viz 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.
2019MNRAS.487.2977G viz 17       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 viz 17       D               1 5696 27 Runaway young stars near the Orion Nebula. McBRIDE A. and KOUNKEL M.

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