Maps of the 36 GHz methanol emission (Liechti+, 1996)

Details Maps of the 36 GHz methanol emission (Liechti+, 1996) Maps of the 36 GHz methanol emission (Liechti+, 1996)

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..33140615l&link_type=abstract

VizieR On-line Data Catalog: J/A+A/314/615. Originally published in: 1996A&A...314..615L

Other

Masers

Scientific paper

We have used the Effelsberg 100-meter telescope to map the 36GHz 4-1->30E methanol transition in galactic star forming regions where methanol masers were previously detected. In most sources, the emission consists in one or several narrow (maser) features superimposed on a broader, presumably quasi-thermal component. The line shapes and positions of the narrow features are often similar to those observed in the other ClassI methanol maser transitions (at 25, 44, 84 and 95GHz), but with some exceptions. Our observations confirm that, unlike the strong ClassII methanol masers (at 12.2, and 6.6GHz), the ClassI methanol masers are offset from the compact HII regions, infrared sources and OH/H2O masers. In outflow sources, these are located at the edge of the molecular lobes. (4 data files).

Affiliated with

Also associated with

No associations

Rating

Maps of the 36 GHz methanol emission (Liechti+, 1996) 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 Maps of the 36 GHz methanol emission (Liechti+, 1996), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Maps of the 36 GHz methanol emission (Liechti+, 1996) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1109078