CO J=3-2 observations of M 17 - The interaction of an expanding shock front with molecular clouds

Details CO J=3-2 observations of M 17 - The interaction of an expanding shock front with molecular clouds CO J=3-2 observations of M 17 - The interaction of an expanding shock front with molecular clouds

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...171..252r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 171, no. 1-2, Jan. 1987, p. 252-260. MOESC-supported research.

Astronomy and Astrophysics

Astrophysics

27

Carbon Monoxide, Emission Spectra, Molecular Clouds, Shock Fronts, Astronomical Maps, Astronomical Models, Astronomical Spectroscopy, H Ii Regions, Line Shape, Star Formation, Velocity Distribution

Scientific paper

A study is reported of M 17 (the Omega Nebula, NGC 6618), which is a bright H II region and area of active star formation. An area extending over about 9 x 12 arcmin of the molecular cloud has been mapped in the J=3-2 transition of CO. The CO emission is observed to come mainly from two bars which lie just outside the area of ionized gas. The most intense emission is from the area around the M 17 SW cloud core in the southwest bar. The spectra observed are complex, often showing considerable variation in line shape over small distances. The velocity structure of this region is interpreted as arising from an ensemble of molecular cloud fragments in addition to extended emission. There is an area of star formation to the east of the M 17 SW cloud core, close to the interface between the ionized gas and the molecular cloud.

Affiliated with

Also associated with

No associations

Rating

CO J=3-2 observations of M 17 - The interaction of an expanding shock front with molecular clouds does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with CO J=3-2 observations of M 17 - The interaction of an expanding shock front with molecular clouds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CO J=3-2 observations of M 17 - The interaction of an expanding shock front with molecular clouds will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1621338