The physics and chemistry of dark molecular clouds: A detailed study of L134N

Details The physics and chemistry of dark molecular clouds: A detailed study of L134N The physics and chemistry of dark molecular clouds: A detailed study of L134N

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phdt........19s&link_type=abstract

Ph.D. Thesis Massachusetts Univ., Amherst.

Astronomy and Astrophysics

Astronomy

29

Dark Matter, Line Spectra, Molecular Clouds, Molecular Gases, Radio Astronomy, Abundance, Carbon Monoxide, Density Distribution, Spectrum Analysis, Star Formation

Scientific paper

The dark molecular cloud L134N was studied in detail through radio astronomical observations of spectral lines at millimeter and centimeter wavelengths. A chemical and physical model for L134N, which may be applicable to other dark clouds, was studied to provide insight into the formation of low mass stars and solar systems. The large scale structure of L134N was observed by mapping the C(13)O J= 1-0 spectral line over 1.3 square degrees on the sky. L134N contains approx. 190 solar masses of molecular gas distributed in four subclouds, one of which appears to be rotating.

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