Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-02T19:46:40.016Z Has data issue: false hasContentIssue false
  • English
  • Français

Large–scale and high–sensitivity multi–line CO surveys toward the Galactic center

Published online by Cambridge University Press:  22 May 2014

R. Enokiya ,
K. Torii ,
M. Schultheis ,
Y. Asahina ,
R. Matsumoto ,
H. Yamamoto ,
K. Tachihara ,
T. Okuda ,
M. R. Morris  and
Y. Fukui
R. Enokiya
Affiliation:
Department of Physics and Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi, 464-8601, Japan email: [email protected]
K. Torii
Affiliation:
Department of Physics and Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi, 464-8601, Japan email: [email protected]
M. Schultheis
Affiliation:
Observatoire de la Cote d'Azur Laboratoire Lagrange, CNRS UMR 7293, B. P. 4229 06304 Nice Cedex 04, France
Y. Asahina
Affiliation:
Faculty of Science, Chiba University, Inage-ku, Chiba 263-8522
R. Matsumoto
Affiliation:
Faculty of Science, Chiba University, Inage-ku, Chiba 263-8522
H. Yamamoto
Affiliation:
Department of Physics and Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi, 464-8601, Japan email: [email protected]
K. Tachihara
Affiliation:
Department of Physics and Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi, 464-8601, Japan email: [email protected]
T. Okuda
Affiliation:
National Astronomical Observatory of Japan, Mitaka, Tokyo, 181-8588, Japan
M. R. Morris
Affiliation:
Department of Physics and Astronomy, University of California, Los Angeles, California 90095-1547, USA
Y. Fukui
Affiliation:
Department of Physics and Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi, 464-8601, Japan email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We carried out large–scale (4 × 2 degree) CO multi–line observations toward the central molecular zone (CMZ) in the Galactic center (GC) with the NANTEN2 4m telescope and mapped several diffuse molecular features located at relatively high Galactic latitudes above 0°.6. These high–latitude features are composed of diffuse molecular halo gas and molecular filaments according to their morphological aspects. Their high velocities and high intensity ratios between 12CO J = (2−1) and J = (1−0) clearly indicate their location in the GC, and their total mass amount to ∼10% of that of the CMZ. We discuss that magnetic field is a possible mechanism of these high–latitude molecular features lifting up toward high galactic latitude.

Keywords

ISM: clouds — Radio lines: ISM — Galaxy: Galactic center
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. 194 - 198
Copyright
Copyright © International Astronomical Union 2014 

References

Crocker, R. M., Jones, D. I., Melia, F.et al. 2010, Science 463, 65Google Scholar
Enokiya, R., Torii, K., Schultheis, M.et al. 2013, Astro-ph 1310, 8229Google Scholar
Fukui, Y., Yamamoto, H., Fujishita, M.et al. 2006, Science 314, 106Google Scholar
LaRosa, T. N., Nord, M. E., Lazio, T. J. W.et al. 2004, ApJS 607, 302Google Scholar
Machida, M., Matsumoto, R., Nozawa, S.et al. 2009, PASJ 440, 308Google Scholar
Morris, M. R. & Serabyn, E. 1996, ARA&A 34, 645Google Scholar
Morris, M. R., Uchida, K., & Do, T. 2006, Nature 440, 308CrossRefGoogle Scholar
Oka, T., Hasegawa, T., Sato, F.et al. 1998, ApJS 118, 455CrossRefGoogle Scholar
Parker, E. N. 1966, ApJ 145, 811CrossRefGoogle Scholar
Sofue, Y. 2007, PASJ 59, 189CrossRefGoogle Scholar
Stolovy, S., Ramirez, S., Arendt, R. G.et al. 2006, JPhCS 54, 176Google Scholar
Torii, K., Kudo, N., Fujishita, M., et al. 2010, PASJ 62, 1307Google Scholar
Torii, K., Enokiya, R., Fukui, Y.et al. 2013, in IAU Symp. 303, The Galactic Center: Feeding and Feedback in a Normal Galactic NucleusGoogle Scholar
Tsuboi, M. & Handa, T. 2010, ApJ 719, 177CrossRefGoogle Scholar
Uchida, K. I., Morris, M. R., Serabyn, E., et al. 1994, ApJ 421, 505CrossRefGoogle Scholar
Yusef-Zadeh, F., Morris, M. R., & Chance, D. 1984, Nature 310, 557Google Scholar