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The warm ISM in the Sgr A region: mid-J CO, atomic carbon, ionized atomic carbon, and ionized nitrogen line observations with the Herschel/HIFI and NANTEN2/SMART Telescopes

Published online by Cambridge University Press:  22 May 2014

Pablo García ,
Robert Simon ,
Jürgen Stutzki ,
Miguel Requena-Torres ,
Rolf Güsten ,
Yasuo Fukui ,
Hiroaki Yamamoto ,
Frank Bertoldi ,
Michael Burton  and
Leonardo Bronfman
...Show all authors
Pablo García
Affiliation:
I. Physikalisches Institut der Universität zu Köln D-50937, Cologne, Germany email: [email protected]
Robert Simon
Affiliation:
I. Physikalisches Institut der Universität zu Köln D-50937, Cologne, Germany email: [email protected]
Jürgen Stutzki
Affiliation:
I. Physikalisches Institut der Universität zu Köln D-50937, Cologne, Germany email: [email protected]
Miguel Requena-Torres
Affiliation:
Max-Plank-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
Rolf Güsten
Affiliation:
Max-Plank-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
Yasuo Fukui
Affiliation:
Nagoya University, Japan
Hiroaki Yamamoto
Affiliation:
Nagoya University, Japan
Frank Bertoldi
Affiliation:
Universität Bonn, Germany
Michael Burton
Affiliation:
University of New South Wales, Australia
Leonardo Bronfman
Affiliation:
Universidad de Chile, Chile
Hideo Ogawa
Affiliation:
Osaka Prefecture University, Japan
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Abstract

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We present Herschel/HIFI sub-mm atomic carbon ([Ci] 3P1 – 3P0 and [Ci] 3P2 – 3P1), ionized carbon ([Cii] 2P3/2 – 2P1/2), and ionized nitrogen ([Nii] 3P1 – 3P0) line observations obtained in the frame of the Herschel Guaranteed Time HEXGAL (Herschel EXtraGALactic) key program (P. I. Rolf Güsten, MPIfR), and NANTEN2/SMART carbon monoxide (CO(J = 4 – 3)) observations of the warm gas around the Sgr A region. The spectrally resolved emission from all lines, and the corresponding line intensity ratios, show a very complex morphology. The determination of spatial and spectral (anti)correlation with known sources in the Sgr A region such as the Arched Filaments, NTF filaments, the Sickle, Quintuplet cluster, CND clouds, is ongoing work.

Keywords

Galaxy: centerISM: cloudssubmillimeter
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. 73 - 74
Copyright
Copyright © International Astronomical Union 2014 

References

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