Methanol masers: tracers of outflows?

Details Methanol masers: tracers of outflows? Methanol masers: tracers of outflows?

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001evn5.proc..178m&link_type=abstract

Proceedings of the 5th European VLBI Network Symposium, Chalmers University of Technology, Gothenburg, Sweden, eds. J.E. Conway,

Computer Science

Star: Formation, Maser, Circumstellar Matter, Hii Region, Techniques: Interferometric

Scientific paper

We have evidence that some 6.7 and 12.2 GHz methanol masers may trace outflows emerging from protostars. The methanol masers could trace either well collimated outflows or more randomly distributed clumps formed by ionised stellar winds. We present preliminary proper motion studies of 12.2 GHz methanol masers. First results show that the proper motions of the maser components in G 9.62+0.20 are consistent with masers forming in an outflow rather than a disk.

Affiliated with

Also associated with

No associations

Rating

Methanol masers: tracers of outflows? 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 Methanol masers: tracers of outflows?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Methanol masers: tracers of outflows? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-923838