| Literature DB >> 17023654 |
Yasuo Fukui1, Hiroaki Yamamoto, Motosuji Fujishita, Natsuko Kudo, Kazufumi Torii, Satoshi Nozawa, Kunio Takahashi, Ryoji Matsumoto, Mami Machida, Akiko Kawamura, Yoshinori Yonekura, Norikazu Mizuno, Toshikazu Onishi, Akira Mizuno.
Abstract
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 (12)CO (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.Year: 2006 PMID: 17023654 DOI: 10.1126/science.1130425
Source DB: PubMed Journal: Science ISSN: 0036-8075 Impact factor: 47.728