Discovery of water vapor maser in the large Magellanic cloud

Details Discovery of water vapor maser in the large Magellanic cloud Discovery of water vapor maser in the large Magellanic cloud

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980stin...8120995s&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Magellanic Clouds, Masers, Radio Astronomy, Spectrum Analysis, Water Vapor, Emission Spectra, H Lines, Molecular Spectra, Nebulae, Radial Velocity

Scientific paper

A large scale survey for detection of water vapor sources in the Large Magellanic Cloud, with use of a maser amplifier at Itapetinga Radio Observatory, led to the discovery of a source associated to N159 with line features of intensity of 7.2 Jy (233.6kms/1) and 3.2 Jy (213.9 km/s) (detection limits of the order of 1 Jy). The other molecules found in the direction of N159 have radial velocities nearly coincident.

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