The distribution of extinction in the dark cloud complex L1295 as derived from general star counts

Details The distribution of extinction in the dark cloud complex L1295 as derived from general star counts The distribution of extinction in the dark cloud complex L1295 as derived from general star counts

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aj.....90..308r&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 90, Feb. 1985, p. 308, 309.

Astronomy and Astrophysics

Astronomy

2

Interstellar Extinction, Molecular Clouds, Star Distribution, Astronomical Maps, Filaments, Photographic Plates

Scientific paper

The distribution of extinction in the dark cloud complex L1295 has been derived from general star counts covering an area of 12.5 deg2. The complex appears to have a generally filamentary structure. Several clouds are observed to be embedded along two ridge-like structures. A total mass of 9300 M_sun; is observed in the complex. Two small, very dense clouds, approximately 1 pc in diameter, and with densities greater than 5600 H I/cm3, have been detected.

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