A molecular study of the dark clouds L 1506 and L 1529 in Taurus

Details A molecular study of the dark clouds L 1506 and L 1529 in Taurus A molecular study of the dark clouds L 1506 and L 1529 in Taurus

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...189..207n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 189, no. 1-2, Jan. 1988, p. 207-220.

Astronomy and Astrophysics

Astrophysics

19

Astronomical Spectroscopy, Emission Spectra, Interstellar Matter, Molecular Clouds, Taurus Constellation, Abundance, Carbon Monoxide, Photochemical Reactions, Spectral Resolution

Scientific paper

The authors have surveyed at moderate resolution (5arcmin) the 13CO (J = 1-0) emission of the Taurus dark clouds L 1529 and L 1506. The data together with the visual extinction Av derived from star counts, give two values of the 13CO abundance. The masses of L 1529 and L 1506 are found to be 700 and 460 M_sun; respectively. The mean density is 400 cm-3 for both clouds. The 13CO abundance show variations from place to place across the whole Taurus-Auriga-Perseus complex. The velocity structure of the region is found to be very confused. The gravitational stability of the clouds is examined.

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