Targets for Future Southern mm-VLBI Experiments from the Mopra SiO Line Survey

Details Targets for Future Southern mm-VLBI Experiments from the Mopra SiO Line Survey Targets for Future Southern mm-VLBI Experiments from the Mopra SiO Line Survey

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..340..404c&link_type=abstract

Future Directions in High Resolution Astronomy: The 10th Anniversary of the VLBA, ASP Conference Proceedings, Vol. 340. Edited

Astronomy and Astrophysics

Astronomy

Scientific paper

A survey has been made in the SiO J=2-1 (ν=1) transition at 86.243 GHz and J=2-1 (ν=0) transition at 86.846 GHz with the Mopra radiotelescope and the SEST telescope for color-selected IRAS sources in the galactic disk with detected OH maser emission. A comparison between NVSS survey images show that radio continuum sources are spatially associated with radio positions of the brightest SiO masers. A few sources show hot blackbody temperatures with T>300 K and broad thermal wings are seen underlying the main SiO maserline at 3 mm.

Affiliated with

Also associated with

No associations

Rating

Targets for Future Southern mm-VLBI Experiments from the Mopra SiO Line Survey 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 Targets for Future Southern mm-VLBI Experiments from the Mopra SiO Line Survey, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Targets for Future Southern mm-VLBI Experiments from the Mopra SiO Line Survey will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1032779