Synergy of multifrequency studies from observations of NGC6334I

Details Synergy of multifrequency studies from observations of NGC6334I Synergy of multifrequency studies from observations of NGC6334I

2008-11-15

arxiv.org/abs/0811.2495v1

J.Phys.Conf.Ser.131:012030,2008

Astronomy and Astrophysics

Astrophysics

6 pages, 6 figures, appeared in the proceedings of the workshop 'The Universe Under The Microscope - Astrophysics At High Angu

Scientific paper

10.1088/1742-6596/131/1/012030

We combine multifrequency observations from the millimeter to near infrared wavelengths that demonstrate the spatial distributions of H2, CO, and NH3 emission, which are all manifestations of various shocks driven by outflows of deeply embedded sources in NGC6334I. In addition to the well-known northeast-southwest outflow we detect at least one more outflow in the region by combining observations from APEX, ATCA, SMA, Spitzer and VLT/ISAAC. Potential driving sources will be discussed. NGC6334I exhibits several signs of active star formation and will be a major target for future observatories such as Herschel and ALMA.

Affiliated with

Also associated with

No associations

Rating

Synergy of multifrequency studies from observations of NGC6334I 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 Synergy of multifrequency studies from observations of NGC6334I, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Synergy of multifrequency studies from observations of NGC6334I will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-39361