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Chemical differentiation in Sagittarius B2(N): first high resolution results

Published online by Cambridge University Press:  22 May 2014

J. F. Corby ,
P. A. Jones ,
M. R. Cunningham  and
A. J. Remijan
J. F. Corby
Affiliation:
Dept. of Astronomy, University of Virginia, P. O. Box 400325, Charlottesville, VA 22904, USA email: jfc9va@virginia.edu
P. A. Jones
Affiliation:
School of Physics, University of New South Wales, Sydney NSW 2052, Australia emails: paulcojones@gmail.com, mcunningham@phys.unsw.edu.au
M. R. Cunningham
Affiliation:
School of Physics, University of New South Wales, Sydney NSW 2052, Australia emails: paulcojones@gmail.com, mcunningham@phys.unsw.edu.au
A. J. Remijan
Affiliation:
National Radio Astronomy Observatory, 520 Edgemont Rd, Charlottesville, VA 22903, USA email: aremijan@nrao.edu
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Abstract

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Sgr B2 is an active high mass star forming region in the Galactic center and the pre-eminent interstellar source of organic chemistry. Newly available broad bandwidth radio interferometry data enables a spatially resolved study of the chemical environments within the Sgr B2(N) core. We present selections from a 30 - 50 GHz spectral line survey conducted with the ATCA.

Keywords

astrochemistry – ISM: molecules – individual objects: Sagittarius B2
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S303: The Galactic Center: Feeding and Feedback in a Normal Galactic Nucleus , October 2013 , pp. 205 - 207
Copyright
Copyright © International Astronomical Union 2014 

References

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