EXTENDED SUBMILLIMETER EMISSION OF THE GALACTIC CENTER AND NEAR-INFRARED/SUBMILLIMETER VARIABILITY OF ITS SUPERMASSIVE BLACK HOLE

EXTENDED SUBMILLIMETER EMISSION OF THE GALACTIC CENTER AND NEAR-INFRARED/SUBMILLIMETER VARIABILITY OF ITS SUPERMASSIVE BLACK HOLE

The innermost tens of parsecs of our Galaxy are characterized by the presence of molecular cloud complexes surrounding Sgr A*, the radiative counterpart of the supermassive black hole (~4 × 10[superscript 6] M ☉) at the Galactic center. We seek to distinguish the different physical mechanisms that d...

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Main Authors: Garcia-Marin, M. (Author), Eckart, A. (Author), Weiss, A. (Author), Witzel, G. (Author), Bremer, M. (Author), Zamaninasab, M. (Author), Morris, M. R. (Author), Schodel, R. (Author), Kunneriath, D. (Author), Nishiyama, S. (Author), Baganoff, Frederick K. (Contributor), Dovciak, Michal (Author), Sabha, N. (Author), Duschl, W. J. (Author), Moultaka, J. (Author), Karas, Vladimir (Contributor), Najarro, F. (Author), Muzic, K. (Author), Straubmeier, C. (Author), Vogel, S. N. (Author), Krips, M. (Author), Wiesemeyer, H. (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: Institute of Physics/American Astronomical Society, 2015-03-04T21:19:34Z.
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