ATCA 1.2 cm Observations of the Massive Star Forming Region G305.2+0.2

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

13 pages 11 figures

Scientific paper

We report on Australia Telescope observations of the massive star forming region G305.2+0.2 at 1.2 cm. We detected emission in five molecules towards G305A, confirming its hot core nature. We determined a rotational temperature of 26 K for methanol. A non-LTE excitation calculation suggests a kinematic temperature of order 200 K. A time dependent chemical model is also used to model the gas phase chemistry of the hot core associated with G305A. A comparison with the observations suggest an age of between 2 x10^4 and 1.5 x10^5 years. We also report on a feature to the SE of G305A which may show weak Class I methanol maser emission in the line at 24.933 GHz. The more evolved source G305B does not show emission in any of the line tracers, but strong Class I methanol maser emission at 24.933 GHz is found 3\arcsec to the east. Radio continuum emission at 18.496 GHz is detected towards two \hii regions. The implications of the non-detection of radio continuum emission toward G305A and G305B are also discussed.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

ATCA 1.2 cm Observations of the Massive Star Forming Region G305.2+0.2 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 ATCA 1.2 cm Observations of the Massive Star Forming Region G305.2+0.2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ATCA 1.2 cm Observations of the Massive Star Forming Region G305.2+0.2 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-552946

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.