Distribution of OB stars and absorbing matter in the region of the association per OB1

Details Distribution of OB stars and absorbing matter in the region of the association per OB1 Distribution of OB stars and absorbing matter in the region of the association per OB1

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984afz....20..437g&link_type=abstract

(Astrofizika, vol. 20, May-June 1984, p. 437-445) Astrophysics (ISSN 0571-7132), vol. 20, no. 3, Nov. 1984, p. 234-239. Translat

Astronomy and Astrophysics

Astrophysics

7

B Stars, Interstellar Matter, O Stars, Star Distribution, Distance, Stellar Spectrophotometry

Scientific paper

The results are given of spectrophotometric investigation of 86 OB stars in the region of the association Per OB1. The blue (4000-4800 A) absolute spectrophotometric gradients, the color excesses, and the distances of these stars were determined. Analysis of the obtained results makes it possible to draw the following conclusions: (1) the centers of the OB clusters h and Chi Per apparently have a separation of about 1000 parsec along the line of sight; (2) the absorbing matter in the direction of the association Per OB1 is concentrated in the regions occupied by the OB stars.

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