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- W31180328 abstract "Background. The existence of the young stellar group Bochum 7 (l = 265◦, b = -2◦) was indicated by Moffat & Vogt (1975, A&AS 20, 85). They suggested that several OB stars from the LSS catalog around WR 12 may be an OB association at 5.8kpc. Young open clusters and OB associations are very important objects for understanding the underlying star formation processes as well as studying the spiral structure of the Galaxy. In this way, Bochum 7 could give some information on the spiral structure of the outer region. Lundstrom & Stenholm (1984, A&AS 58, 163) proposed that Bo 7 is an OB association of ∼ 30 pc of size. Sung et al. (1999, JKAS 32, 109) suggested that the stars associated with Bo 7 are only a local concentration in the density of young stars belonging to the Vel OB3 association." @default.
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- W31180328 date "2003-01-01" @default.
- W31180328 modified "2023-09-26" @default.
- W31180328 title "New Members of the Galactic OB Association Bochum7" @default.
- W31180328 hasPublicationYear "2003" @default.
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