A search for 183 GHz emission from water in late-type stars

Details A search for 183 GHz emission from water in late-type stars A search for 183 GHz emission from water in late-type stars

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...286..310k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 286, Nov. 1, 1984, p. 310-313. NASA-supported research. Previously announce

Astronomy and Astrophysics

Astronomy

6

Airborne Equipment, Astronomy, Late Stars, Line Spectra, Masers, Spectrum Analysis, Water Vapor, Abundance, Fast Fourier Transformations, Prediction Analysis Techniques, Semiregular Variable Stars, Thermal Emission, Tracking (Position)

Scientific paper

A search was made for 183 GHz line emission from water vapor in the direction of twelve Mira and two semiregular variables. Upper limits to the emission are in the range of 2000 to 5000 Jy. It is estimated that thermal emission from the inner regions of late type stellar envelopes will be on the order of ten Jy. Maser emission, according to one model, would be an order of magnitude stronger. From the limited set sampled, the possibility of very strong maser emission at 183 GHz cannot yet be ruled out.

Affiliated with

Also associated with

No associations

Rating

A search for 183 GHz emission from water in late-type stars 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 A search for 183 GHz emission from water in late-type stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A search for 183 GHz emission from water in late-type stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1751477