Investigation of diffuse-matter distribution in the star-formation region in Taurus

Details Investigation of diffuse-matter distribution in the star-formation region in Taurus Investigation of diffuse-matter distribution in the star-formation region in Taurus

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kfnt....1...80l&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 1, Jan.-Feb. 1985, p. 80-87. In Russian.

Computer Science

Crab Nebula, Extraterrestrial Matter, Mass Distribution, Molecular Clouds, Star Formation, Taurus Constellation, Carbon Monoxide, Cosmic Dust, Density Distribution, Spectrum Analysis

Scientific paper

The dust distribution in the region centered at alpha(1950) = 4 h 3 m, delta = +26 deg is studied. The density maximum of absorbing material is located at a distance from 50 to 200 pc. A dark cloud is located in the central part of the star-formation region at a distance of 125 pc; the cloud size is 20 x 10 pc. The cloud is very patchy and appears to be a complex of dark nebulae. The lower limit of the total mass of the dark-cloud material is approximately 2000 solar masses. A correlation is found between the location of the dust cloud and the densest part of the CO cloud.

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