The structure and dynamics of M17SW

Details The structure and dynamics of M17SW The structure and dynamics of M17SW

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.216..159h&link_type=abstract

Astrophysics and Space Science, vol. 216, no. 1-2, p. 159-160

Astronomy and Astrophysics

Astrophysics

1

Carbon Monoxide, Gas Dynamics, Infrared Stars, Interstellar Gas, Molecular Clouds, Protostars, Star Formation, B Stars, Emission Spectra, Line Spectra, Masers, Molecular Spectra, O Stars, Stellar Gravitation

Scientific paper

The M17SW molecular cloud core has been mapped at high resolution in the C(17)O J = 3 approaches 2 transition and in 450, 600, 800, 1100, and 1300 micron continuum emission, using the JCMT. The clumpy nature of the cloud core is clearly revealed and the northern condensation has been resolved into 3 main clumps, each of which lies close to an H2O maser, suggesting that they may contain young embedded stellar objects.

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