Possible CO clouds interacting with the SNRs G21.8-0.6 and G32.8-0.1

Details Possible CO clouds interacting with the SNRs G21.8-0.6 and G32.8-0.1 Possible CO clouds interacting with the SNRs G21.8-0.6 and G32.8-0.1

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007iaus..242...66z&link_type=abstract

Astrophysical Masers and their Environments, Proceedings of the International Astronomical Union, IAU Symposium, Volume 242, p.

Mathematics

Logic

Ism:Clouds, Ism: Individual (G21.8-0.6, G32.8-0.1), Ism:Molecules, Masers, Supernova Remnants

Scientific paper

We have obtained the first CO(1-0) maps towards the SNRs G21.8-0.6 and G32.8-0.1, which are associated with OH 1720 MHz masers. Based on the morphological correspondence between the radio remnant and the CO cloud, and the velocity and position agreement between the OH maser and CO clouds, we tentatively suggest the clouds may be interacting with G21.8-0.6 and G32.8-0.1. However, the shock-excited line broadening was not obvious for these two SNRs. We discuss the possible reasons for this.

Affiliated with

Also associated with

No associations

Rating

Possible CO clouds interacting with the SNRs G21.8-0.6 and G32.8-0.1 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 Possible CO clouds interacting with the SNRs G21.8-0.6 and G32.8-0.1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Possible CO clouds interacting with the SNRs G21.8-0.6 and G32.8-0.1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-862647