Extinction curves and intrinsic colours in local and distant OB complexes

Details Extinction curves and intrinsic colours in local and distant OB complexes Extinction curves and intrinsic colours in local and distant OB complexes

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...175..186k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 175, no. 1-2, March 1987, p. 186-192.

Astronomy and Astrophysics

Astrophysics

14

B Stars, Interstellar Extinction, Interstellar Matter, O Stars, Stellar Color, Stellar Spectra, Absorption Spectra, Classifying, Galactic Structure, Spectral Energy Distribution, Stellar Models

Scientific paper

The present investigation of extinctions in two different Galactic disk regions is based on stars of (B1 V) Sp/L class, and indicates that the shapes of extinction curves, and perhaps the total/selective absorption ratios, differ among young star complexes. In addition, a small difference is noted among the intrinsic energy distributions in B1 V stars' spectra in the complexes studied. The two associations studied are Sco-Ori and the Perseus arm.

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