Distribution of extinction in the Corona Australis dark cloud complex

Details Distribution of extinction in the Corona Australis dark cloud complex Distribution of extinction in the Corona Australis dark cloud complex

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978aj.....83..234r&link_type=abstract

Astronomical Journal, vol. 83, Mar. 1978, p. 234-240.

Astronomy and Astrophysics

Astronomy

39

Interstellar Extinction, Star Clusters, Astronomical Photography, Error Analysis, Magnetic Field Configurations, Polarization (Waves)

Scientific paper

General star counts have been used over a region of 92 sq deg to derive the photographic extinction due to the dark cloud complex in Corona Australis. The constituent clouds in this complex are found to be systematically distributed in an extensive region of low obscuration. The mass of this extended background material and lower limits on the masses of the embedded clouds have been derived.

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