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=2001crlj...48..105t&link_type=abstract

Journal of the Communications Research Laboratory. Special Issue: Large Aperture Radio Telescopes at Kashima Space Research Cent

Astronomy and Astrophysics

Astronomy

Water Vapor, Masers, Radio Telescopes, Water Masers, Protostars, Point Sources, Late Stars, Color, Infrared Astronomy Satellite

Scientific paper

We carried out an H2O maser survey by using the 34 m radio telescope at Kashima Space Research Center, CRL in Japan. Sources were selected from the IRAS point source catalogue according to their position on the two-color diagram, and included most of the known H2O maser sources associated with late-type stars and proto-stellar objects. From a total of 842 H2O maser candidates, 265 were found to produce H2O maser emissions, and 44 of these constitute new detections.

Affiliated with

Also associated with

No associations

Rating

Water Vapor Maser Survey by Using the Kashima 34m Radio Telescope does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Water Vapor Maser Survey by Using the Kashima 34m Radio Telescope, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Water Vapor Maser Survey by Using the Kashima 34m Radio Telescope will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1006321