The relative positions of the OH and H2O masers in W49N and W3/OH/

Details The relative positions of the OH and H2O masers in W49N and W3/OH/ The relative positions of the OH and H2O masers in W49N and W3/OH/

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...200l.111m&link_type=abstract

Astrophysical Journal, vol. 200, Sept. 1, 1975, pt. 2, p. L111-L114.

Astronomy and Astrophysics

Astronomy

24

Hydroxyl Emission, Interstellar Masers, Interstellar Matter, Microwave Spectra, Molecular Spectra, Water Vapor, Electron Transitions, Emission Spectra, Line Spectra, Maser Outputs, Radio Sources (Astronomy)

Scientific paper

The relative positions of the OH and H2O masers in W49N and W3(OH) have been found by simultaneously observing both masering transitions with a very-long-baseline interferometer. In both sources, the OH and H2O features are clearly separated and occupy two distinct regions of space, separated by 48,000 AU and 18,000 AU in W49N and W3(OH), respectively. The two masering regions appear unlikely to have the same source of excitation.

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