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ReportsMolecular Loops in the Galactic Center: Evidence for Magnetic Flotation
The central few hundred parsecs of the Milky Way host a massive black hole and exhibit very violent gas motion and high temperatures in molecular gas. The origin of these properties has been a mystery for the past four decades. Wide-field imaging of the 12CO (rotational quantum number J = 1 to 0) 2.6-millimeter spectrum has revealed huge loops of dense molecular gas with strong velocity dispersions in the galactic center. We present a magnetic flotation model to explain that the formation of the loops is due to magnetic buoyancy caused by the Parker instability. The model has the potential to offer a coherent explanation for the origin of the violent motion and extensive heating of the molecular gas in the galactic center.
1 Department of Astrophysics, Nagoya University, Chikusa-ku, Nagoya 464-8602, Japan.
2 Department of Science, Ibaraki University, 2-1-1 Bunkyo, Mito, Ibaraki 310-8512, Japan. 3 National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan. 4 The Graduate University for Advanced Studies, Hayama, Miura, Kanagawa, 240-0193, Japan. 5 Department of Physics, Faculty of Science, Chiba University, 1-33, Yayoi-cho, Inage-ku, Chiba 263-8522, Japan. 6 Department of Physical Science, Osaka Prefecture University, 1-1 Gakuen-cho, Sakai, Osaka 599-8531, Japan. 7 Solar-Terrestrial Environment Laboratory, Nagoya University, Chikusaku, Nagoya, 464-8601, Japan. * To whom correspondence should be addressed. E-mail: fukui{at}a.phys.nagoya-u.ac.jp
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Science. ISSN 0036-8075 (print), 1095-9203 (online)