Dissipative structures of diffuse molecular gas (Hily-Blant+ 2007)

Details Dissipative structures of diffuse molecular gas (Hily-Blant+ 2007) Dissipative structures of diffuse molecular gas (Hily-Blant+ 2007)

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34690173h&link_type=abstract

VizieR On-line Data Catalog: J/A+A/469/173. Originally published in: 2007A&A...469..173H

Physics

Interstellar Medium, Radio Lines, Carbon Monoxide

Scientific paper

These maps are part of a large project aimed at analyzing the small scale morphology and velocity structure of the parsec-scale environment of a low mass dense core. The Polaris field is translucent and shows no signpost of star formation, therefore allowing an analysis of a purely turbulent field prior to star formation. Our work is based on large maps made with the IRAM-30m telescope in the two lowest rotational transitions of 12CO and 13CO (1-0) with high angular (20" or 0.015pc at 115GHz) and spectral (0.055km/s) resolutions. The new data superseeds the first IRAM Key-project of Falgarone et al. (1998A&A...331..669F, Cat. ).
The field is centered at 02:00:06.0-87:42:04.1 (J2000); at the estimated distance of 150pc, the size of the maps are 0.72*0.55pc2.
(1 data file).

Affiliated with

Also associated with

No associations

Rating

Dissipative structures of diffuse molecular gas (Hily-Blant+ 2007) 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 Dissipative structures of diffuse molecular gas (Hily-Blant+ 2007), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dissipative structures of diffuse molecular gas (Hily-Blant+ 2007) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1721461