Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...139..317g&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 139, no. 2, Oct. 1984, p. 317-329.
Astronomy and Astrophysics
Astronomy
34
Cassiopeia A, Formaldehyde, Molecular Clouds, Radio Astronomy, Absorption Spectra, Carbon Monoxide, Centimeter Waves, Continuous Spectra, Optical Thickness
Scientific paper
The 6 cm 110 - 111 H2CO absorption in the Perseus arm feature in the direction of Cas A has been mapped with the Westerbork Synthesis Radio Telescope (WSRT). Only a small part of Cas A is absorbed. In agreement with the 2 cm 211-212 results of Batrla et al. (1983), there is no H2CO absorption in the northern half of Cas A. The low optical depths measured with single dish telescopes (≤0.06) are due to small filling factors in a clumpy medium. With higher angular resolution optical depths of ≡1 are observed. These clumps have H2 densities of ≡104cm-3, sizes in the range 0.1 - 0.4 pc and total masses in the range 0.2 - 66 M_sun;. A comparison with CO and H I absorption observations has been carried out. Twelve of the H2CO clumps have possible H I counterparts.
Dickel Helene R.
Goss William Miller
Kalberla Peter M. W.
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