V* V855 Ori , the SIMBAD biblio

V* V855 Ori , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST12:24:24


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Title First 3 Authors
1965VA......8...89H 190 ~ Flare stars in stellar aggregates of different ages. HARO G. and CHAVIRA E.
1970IBVS..480....1K 2217 35 57th Name-list of variable stars KUKARKIN B.V., KHOLOPOV P.N. and PEROVA N.B.
1992A&A...265..144W 157 9 Emission-line stars in L 1641. WOUTERLOOT J.G.A. and BRAND J.
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 15       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 15       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.
2014A&A...570A..30P viz 15       D               1 1688 4 Hα emission-line stars in molecular clouds. II. The M 42 region. PETTERSSON B., ARMOND T. and REIPURTH B.
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.
2019AJ....158..122K viz 16       D               1 290057 150 Untangling the Galaxy. I. Local structure and star formation history of the Milky Way. KOUNKEL M. and COVEY K.
2019ApJ...884....6M viz 16       D               1 5695 27 Runaway young stars near the Orion Nebula. McBRIDE A. and KOUNKEL M.
2022ApJS..262....7H viz 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.
2023A&A...674A..21M viz 17       D               1 11510 8 Gaia Data Release 3 Validating the classification of variable young stellar object candidates. MARTON G., ABRAHAM P., RIMOLDINI L., et al.

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