Water Vapor Maser Survey by Using the Kashima 34m Radio Telescope

Details Water Vapor Maser Survey by Using the Kashima 34m Radio Telescope Water Vapor Maser Survey by Using the Kashima 34m Radio Telescope

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001crlrv..47..107t&link_type=abstract

Review of the Communications Research Laboratory, vol. 47, p. 107

Astronomy and Astrophysics

Astronomy

Water Vapor, Water Masers, Surveys, Late Stars, Color, Infrared Astronomy Satellite, Japan, Masers, Losses, Radio Telescopes

Scientific paper

We carried out an H2O maser survey by using the 34-m radio telescope at the Kashima Space Research Center, CRL in Japan. Sources were selected from the IRAS point-source catalogue by their position on the two-color diagram; most of all known H2O maser sources associated with late-type stars and proto-stellar objects were included. Of the 842 H2O maser candidates surveyed, 265 sources had H2O maser emissions, and 44 sources were newly detected.

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