A methanol line survey toward high-mass star-forming regions

Details A methanol line survey toward high-mass star-forming regions A methanol line survey toward high-mass star-forming regions

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...387..179m&link_type=abstract

Astronomy and Astrophysics, v.387, p.179-186 (2002)

Astronomy and Astrophysics

Astrophysics

16

Masers, Stars: Formation, Stars: Circumstellar Matter

Scientific paper

We present the results of a search for methanol maser and thermal lines in 11 transitions in the range 85-112 GHz toward 23 star-forming regions exhibiting class I and class II methanol masers. The selected frequencies are 85.5, 86.6, 94.5, 95.1, 96.7 (quartet line series), 107.0, 108.8 and 111.2 GHz. Five masers were confirmed at 107.0 GHz while new masers were found at 85.5, 86.6 and 108.8 GHz. Many detected emission lines have a quasi-thermal origin. The detection rates of methanol emission are high at 95.1 GHz (87%) and 96.7 GHz (96%), satisfactory at 107.0 and 108.9 GHz ( ~ 50%) while the detection rates at 85.5, 94.5 and 111.3 GHz are low ( ~ 20%). Most reported 95.1 GHz emission is masing. Table A1 and Figs. A1-A2 of Appendix are only available in electronic form at http://www.edpsciences.org

Affiliated with

Also associated with

No associations

Rating

A methanol line survey toward high-mass star-forming regions 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 methanol line survey toward high-mass star-forming regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A methanol line survey toward high-mass star-forming regions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1716888