The inner galactic structure traced by molecular clouds associated with Ultra-compact HII regions

Details The inner galactic structure traced by molecular clouds associated with Ultra-compact HII regions The inner galactic structure traced by molecular clouds associated with Ultra-compact HII regions

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..34..127l&link_type=abstract

IV Reunión sobre Astronomía Dinámica en Latino América (Eds. C. Allen, A. Ruelas, & R. Teixeira) Revista Mexicana de Astronomía

Astronomy and Astrophysics

Astronomy

Galaxy: Disk, Hii Regions

Scientific paper

We are testing a method to solve for the distances of a sample of ultra-compact (UC) HII regions with IRAS colors and CS(J=2-1) detection. The ambiguity in their kinematical distances is solved using Monte-Carlo simulations. We simulated heliocentric longitude-Radius (l-R) on Galactic plane distributions, and their respective longitude-Velocity_{LSR} (l-V_{LSR}) projections using synthetic associated molecular clouds. The best Galactic distribution is selected by comparison with observed CO maps. Preliminary results for the Galactic quadrant IV are presented.

Affiliated with

Also associated with

No associations

Rating

The inner galactic structure traced by molecular clouds associated with Ultra-compact HII 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 The inner galactic structure traced by molecular clouds associated with Ultra-compact HII regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The inner galactic structure traced by molecular clouds associated with Ultra-compact HII regions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-795686