OH circumstellar masers in association with IRAS sources

Details OH circumstellar masers in association with IRAS sources OH circumstellar masers in association with IRAS sources

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...168..374s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 168, no. 1-2, Nov. 1986, p. 374-376.

Astronomy and Astrophysics

Astronomy

19

Hydroxyl Emission, Infrared Astronomy Satellite, Infrared Stars, Interstellar Masers, Stellar Color, Stellar Envelopes, Infrared Sources (Astronomy), Planetary Nebulae, Radio Sources (Astronomy)

Scientific paper

Because of their far-infrared colors, most sources of the IRAS circulars 8 and 9 were suspected to be OH/IR objects, and observations have been made with Effelsberg and Arecibo radiotelescopes to confirm this nature. This study has been completed with the Nancay radiotelescope; four new objects have been detected. A compilation of the results about this sample is presented. Using these results and an analysis of IRAS data from other types of infrared sources, the possibility of identifying OH/IR stars by their (25-12) micron, (60-25) micron colors is discussed.

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