H2O masers in W49N. I - Maps

Details H2O masers in W49N. I - Maps H2O masers in W49N. I - Maps

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...255..128w&link_type=abstract

Astrophysical Journal, Part 1, vol. 255, Apr. 1, 1982, p. 128-142. Research supported by the Owens Valley Radio Observatory, Co

Astronomy and Astrophysics

Astronomy

62

Astronomical Maps, Interstellar Matter, Nebulae, Water Masers, H Ii Regions, Hydrogen Ions, Power Spectra, Radiant Flux Density, Radio Sources (Astronomy), Stellar Evolution

Scientific paper

Multiple point fringe rate mapping of the H2O masers found in the H II region W49N is presented. The masers were observed with the three-element interferometer consisting of the Haystack 37-m, the National Radio Astronomy Observatory 43-m, and the Owens Valley Radio Observatory 40-m telescopes. The resulting map contains 386 separate features separated by up to 4.0 arcsec. Positive and negative high-velocity features are well separated, and isolated features are found outside the centers of activity noted in earlier observations. The data suggest the entire region to be excited by a single star, with the clusters of features representing the interaction of material accelerated by the star up to velocities of up to a few hundred km/sec with a surrounding stationary or slowly moving medium.

Affiliated with

Also associated with

No associations

Rating

H2O masers in W49N. I - Maps 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 H2O masers in W49N. I - Maps, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and H2O masers in W49N. I - Maps will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-840548