A molecular survey of the dark cloud L 1495 in Taurus

Details A molecular survey of the dark cloud L 1495 in Taurus A molecular survey of the dark cloud L 1495 in Taurus

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...89..421k&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 89, no. 3, Sept. 1991, p. 421-428.

Astronomy and Astrophysics

Astrophysics

9

Interstellar Matter, Molecular Clouds, Rotational Spectra, Carbon Dioxide, Carbon 12, Carbon 13, Gravitational Fields, Millimeter Waves, Stellar Mass, Telescopes

Scientific paper

A molecular survey of L 1495, a nearby dark cloud in Taurus, has been carried out in the J = 1-0 transition of (C-12)O, (C-13)O, and C(O-18) with the University of Cologne 3-m telescope on Gornergrat. The analysis of the data shows that L 1495 can be divided into three major fragments and three smaller parts. Depending on the calculation method, the mass of the whole 3 deg-squared region is estimated to range between 1500 and 2700 solar masses. The average density is 550/cu cm. It is suspected that the fragments as well as the whole cloud are gravitationally bound.

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