Distances of molecular cloud (May+, 1997)

Details Distances of molecular cloud (May+, 1997) Distances of molecular cloud (May+, 1997)

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ycat..33270325m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/327/325. Originally published in: 1997A&A...327..325M

Physics

Molecular Clouds, Carbon Monoxide

Scientific paper

We have used a deep CO survey (at 115GHz) of the third galactic quadrant (May et al., 1993A&AS...99..105M) to derive the physical properties of molecular clouds in the outer Galaxy. Within the range of this survey, from 194° to 270° in galactic longitude, 177 molecular clouds have been identified beyond 2 kpc from the Sun. Distances have been determined kinematically using the rotation curve of Brand (1986, Ph.D. Thesis, University of Leiden) with R&sun;=8.5kpc and Θ&sun;=220km/s. (1 data file).

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