An OH mainline maser survey of IRAS circumstellar envelope sources

Details An OH mainline maser survey of IRAS circumstellar envelope sources An OH mainline maser survey of IRAS circumstellar envelope sources

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as...98..245d&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 98, no. 2, p. 245-260.

Astronomy and Astrophysics

Astronomy

19

Asymptotic Giant Branch Stars, Hydroxyl Emission, Infrared Sources (Astronomy), Interstellar Masers, Stellar Envelopes, Infrared Astronomy Satellite, Stellar Evolution

Scientific paper

We present the results of a survey in the OH mainline at 1667 MHz. Because this line is generally weak in the OH/IR stars, systematic surveys of the mainline maser have not been previously performed. A total of 131 sources were detected out of which 108 were previously unknown. The 1667 MHz profile in OH/IR stars is similar in form to that of the 1612 MHz emission, and the relevant maser properties have been measured under the assumption of the habitual radially expanding envelope model for circumstellar envelopes. We show that the mainline maser is still present in circumstellar envelopes with cool (60/25) colors; its detection is, in fact, higher for such colors. Summary detection rates are given.

Affiliated with

Also associated with

No associations

Rating

An OH mainline maser survey of IRAS circumstellar envelope sources 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 An OH mainline maser survey of IRAS circumstellar envelope sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An OH mainline maser survey of IRAS circumstellar envelope sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1368731