OB Stellar Associations in Crux. II. Analysis and Discussion

Details OB Stellar Associations in Crux. II. Analysis and Discussion OB Stellar Associations in Crux. II. Analysis and Discussion

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aj....111..306t&link_type=abstract

Astronomical Journal v.111, p.306

Astronomy and Astrophysics

Astronomy

13

Stars: Early-Type, Ultraviolet: Stars

Scientific paper

On the bases of the Glazar space telescope observations, made at 1640 Å in the area of about 120 sq. in the direction of the Cru OB 1 stellar association, it is shown that there exist several stellar associations in this direction: four B associations at distances of about 140, 400, 600, and 850 pc (of which the first two are not very certain and the last two may compose together into one group) and five 0 associations at distances of 1200, 1500, 2600, 2700, and 4000 pc. It is shown also that the dust matter within stellar associations themselves has clumpy distribution and the space between associations is rather free of dust.

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