Observations of H2O maser emission in the Large Magellanic Cloud

Details Observations of H2O maser emission in the Large Magellanic Cloud Observations of H2O maser emission in the Large Magellanic Cloud

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.205..275w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 205, Oct. 1983, p. 275-279.

Astronomy and Astrophysics

Astronomy

40

Astronomical Spectroscopy, Interstellar Masers, Magellanic Clouds, Water Masers, Continuous Spectra, Emission Spectra, H Ii Regions, Luminous Intensity

Scientific paper

A search for H2O maser emission towards 10 continuum sources in the Large Magellanic Cloud was made with the Parkes radio telescope (beamwidth 1.7 arcmin). Maser emission was detected near three H II regions, including the 30 Doradus nebula; the positions of the main features were estimated with an accuracy of + or - 15 arcsec. The maser luminosities were comparable to the typical value of H2O masers in galactic H II regions. Upper intensity limits for maser emission in the remaining sources were 0.5 Jy. In contrast with previous observations, no emission was detected near N159.

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