A low-detection limit search for OH emission from infrared stars

Details A low-detection limit search for OH emission from infrared stars A low-detection limit search for OH emission from infrared stars

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...220..836f&link_type=abstract

Astrophysical Journal, Part 1, vol. 220, Mar. 15, 1978, p. 836-840.

Astronomy and Astrophysics

Astronomy

20

Hydroxyl Emission, Infrared Stars, Stellar Radiation, Variable Stars, Infrared Astronomy, Line Spectra, Radio Sources (Astronomy), Stellar Envelopes, Stellar Mass Ejection

Scientific paper

We have used the 300 m telescope of the Arecibo Observatory to examine
154 cool luminous stars for 18 cm OH emission. Six of the stars (RU Ari,
R Com, T Com, RX Oph, UU Peg, and RT Vir) were found to show OH
emission. For the stars without OH emission, we have established
detection limits several times smaller than those of previous surveys.

Affiliated with

Also associated with

No associations

Rating

A low-detection limit search for OH emission from infrared 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 low-detection limit search for OH emission from infrared stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A low-detection limit search for OH emission from infrared stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1078647