Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2010-01-28
RAA 2010 Vol. 10 No. 2, pp.151-158
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
8 pages, 4 figures, published in RAA
Scientific paper
10.1088/1674-4527/10/2/006
The mapping observations of CO $J=2-1$, CO $J=3-2$, $^{13}$CO $J=2-1$ and $^{13}$CO $J=3-2$ lines in the direction of IRAS 22506+5944 have been made. The results show that the cores in the $J=2-1$ transition lines have a similar morphology to those in the $J=3-2$ transition lines. Bipolar molecular outflows are verified. The prior IRAS 22506+5944 observations indicated that two IRAS sources and three H$_{2}$O masers were located close to the peak position of the core. One of the IRAS sources may be the driving source of the outflows. In addition, the H$_{2}$O masers may occur in relatively warm environments. The parameters of the dense core and outflow, obtained by the LTE method, indicate that IRAS 22506+5944 is a high-mass star formation region.
Wang Jun-Jie
Xu Jin-Long
No associations
LandOfFree
Submillimeter/millimeter observations of the high-mass star forming region IRAS 22506+5944 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 Submillimeter/millimeter observations of the high-mass star forming region IRAS 22506+5944, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Submillimeter/millimeter observations of the high-mass star forming region IRAS 22506+5944 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-254037