NGC 7538 IRS 1 - Subarcsecond resolution recombination line and (N-15)H3 maser observations

Details NGC 7538 IRS 1 - Subarcsecond resolution recombination line and (N-15)H3 maser observations NGC 7538 IRS 1 - Subarcsecond resolution recombination line and (N-15)H3 maser observations

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...376..608g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 376, Aug. 1, 1991, p. 608-614.

Astronomy and Astrophysics

Astronomy

17

H Ii Regions, Infrared Sources (Astronomy), Interstellar Masers, Ammonia, Line Spectra, Molecular Clouds

Scientific paper

The present imaging of the NGC 7538 IRS 1-associated (N-15)H3 (J, K) = (3, 3) maser emission with 0.2-arcsec resolution shows the strongest such masers, which may be amplifying the strong double-lobe radio continuum core of the IRS 1 H II region, to be concentrated in two regions separated by about 0.2 arcsec. Observations of several hydrogen recombination line transitions indicate that the velocity of the IRS H II region is similar to that of the ambient molecular cloud.

Affiliated with

Also associated with

No associations

Rating

NGC 7538 IRS 1 - Subarcsecond resolution recombination line and (N-15)H3 maser observations 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 NGC 7538 IRS 1 - Subarcsecond resolution recombination line and (N-15)H3 maser observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and NGC 7538 IRS 1 - Subarcsecond resolution recombination line and (N-15)H3 maser observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1725079