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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Bibliographic Details
Main Authors: Garcia-Marin, M., Eckart, A., Weiss, A., Witzel, G., Bremer, M., Zamaninasab, M., Morris, M. R., Schodel, R., Kunneriath, D., Nishiyama, S., Baganoff, Frederick K., Dovciak, Michal, Sabha, N., Duschl, W. J., Moultaka, J., Karas, Vladimir, Najarro, F., Muzic, K., Straubmeier, C., Vogel, S. N., Krips, M., Wiesemeyer, H.
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:en_US
Published: Institute of Physics/American Astronomical Society 2015
Online Access:http://hdl.handle.net/1721.1/95833

Internet

http://hdl.handle.net/1721.1/95833

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