Gas Dynamic in Perseus

Details Gas Dynamic in Perseus Gas Dynamic in Perseus

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.4101s&link_type=abstract

American Astronomical Society Meeting 205, #41.01; Bulletin of the American Astronomical Society, Vol. 36, p.1408

Astronomy and Astrophysics

Astronomy

Scientific paper

As part of the COMPLETE (COordinated Molecular Probe Line Extinction Thermal Emission) survey of star forming regions, targeting Perseus, Ophiuchus, and Serpens, we have obtained a Nyquist sampled map (40" resolution) of the entirety of Perseus in 12CO(1-0) and 13CO(1-0). In addition, we have mapped several cores, with and without stars, in N2H+(1-0) and CS(1-0) with the FCRAO 14m dish. Here we present the first results of the gas dynamics in Perseus from the COMPLETE survey, covering a range of scales from the velocity gradient across the entire molecular cloud to the rotational energy in individual cores.

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