High-velocity molecular gas in the dark cloud L1529

Details High-velocity molecular gas in the dark cloud L1529 High-velocity molecular gas in the dark cloud L1529

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...255l.119l&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 255, Apr. 15, 1982, p. L119-L122.

Astronomy and Astrophysics

Astrophysics

17

Carbon Monoxide, Early Stars, Interstellar Gas, Molecular Clouds, Astronomical Photography, Astronomical Spectroscopy, Line Spectra

Scientific paper

Embedded stars or young stellar objects in the region of the dark cloud L1529 have been identified as probable energy sources responsible for the unusual, 30 km/sec velocity dispersion of the CO wings detected near the cloud's area of dense condensation. The observations of CO and high-excitation molecules in L1529 are consistent with cloud models in which stellar winds play an important part in dark cloud energetics and internal kinematics.

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