The extreme high-velocity H2O maser features in W49N, W51, and Sagittarius B2

Details The extreme high-velocity H2O maser features in W49N, W51, and Sagittarius B2 The extreme high-velocity H2O maser features in W49N, W51, and Sagittarius B2

Nov 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...210..100m&link_type=abstract

Astrophysical Journal, vol. 210, Nov. 15, 1976, pt. 1, p. 100-107.

Astronomy and Astrophysics

Astronomy

49

Emission Spectra, Infrared Astronomy, Interstellar Masers, Radial Velocity, Stellar Evolution, Water Masers, Gravitational Fields, Milky Way Galaxy, Molecular Spectra, O Stars, Radiant Flux Density, Radiation Pressure, Stellar Winds, Water Vapor

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1976ApJ...210..100M

Affiliated with

Also associated with

No associations

Rating

The extreme high-velocity H2O maser features in W49N, W51, and Sagittarius B2 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 The extreme high-velocity H2O maser features in W49N, W51, and Sagittarius B2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The extreme high-velocity H2O maser features in W49N, W51, and Sagittarius B2 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1725099