Heiles Cloud 2 and TMC-1 - A chemical re-interpretation

Details Heiles Cloud 2 and TMC-1 - A chemical re-interpretation Heiles Cloud 2 and TMC-1 - A chemical re-interpretation

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.251..351w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 251, July 15, 1991, p. 351-355.

Astronomy and Astrophysics

Astronomy

26

Molecular Clouds, Star Formation, Stellar Composition, Stellar Mass, Stellar Winds, Carbon Monoxide, Emission Spectra, Infrared Astronomy Satellite, Stellar Models

Scientific paper

The observation-based dynamical models for B5 are applied to other low-mass star-forming regions, and some observational strategies for the regions are suggested. IRAS observations of the Heiles Cloud 2 are described and interpreted to mean that, like B5, the molecular cloud is controlled by low-mass star formation. A cyclic dynamical-chemical model of the cloud is set forth, and observations of C I, C II, and CH emissions in the vicinity of fragment interfaces are proposed to confirm the chemical signatures of the regions.

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