VLBI observations of 12 GHz methanol masers

Details VLBI observations of 12 GHz methanol masers VLBI observations of 12 GHz methanol masers

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...333l..83m&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 333, Oct. 15, 1988, p. L83-L86.

Astronomy and Astrophysics

Astronomy

52

H Ii Regions, Interstellar Masers, Interstellar Matter, Methyl Alcohol, Star Formation, Very Large Scale Integration, Brightness Temperature, Line Spectra, Maser Outputs, Radio Sources (Astronomy)

Scientific paper

Very long baseline interferometric observations of 20 → 3-1E line of interstellar methanol (CH3OH) at 12.1 GHz toward three star-forming regions are reported. Toward the ultracompact H II region W3(OH), the methanol maser emission is found to emanate from multiple compact regions that are projected against the continuum emission. Individual maser spots have sizes of less than 0arcsec.002 (7×1013cm) and brightness temperatures greater than 2×1010K. For NGC 7538 and Cepheus A, the authors have determined absolute positions for one emission feature.

Affiliated with

Also associated with

No associations

Rating

VLBI observations of 12 GHz methanol masers 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 VLBI observations of 12 GHz methanol masers, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and VLBI observations of 12 GHz methanol masers will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1598308