Water vapour masers in envelopes of OH/IR stars close to the Galactic centre

Details Water vapour masers in envelopes of OH/IR stars close to the Galactic centre Water vapour masers in envelopes of OH/IR stars close to the Galactic centre

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...229..165l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 229, no. 1, March 1990, p. 165-170. Research supported by NFR.

Astronomy and Astrophysics

Astrophysics

15

Galactic Nuclei, Infrared Stars, Interstellar Masers, Stellar Envelopes, Water Masers, Emission Spectra, Hydroxyl Emission, Line Spectra, Star Formation, Stellar Luminosity

Scientific paper

The luminosity function of H2O masers in the envelopes of OH/IR stars close to the Galactic center was studied and compared with H2O luminosities of OH/IR stars in the Galactic disk far from the center. No clear difference was found between the two luminosity distributions. Taken into account the small number of sources used and the broadening of the distributions due to the flux variability and the distance uncertainty, no definite conclusions could be drawn.

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