Constraints on the mass accretion rate onto the supermassive black hole of cygnus : A using the Submillimeter Array
We present the first detailed polarimetric studies of Cygnus A at 230 GHz with the Submillimeter Array (SMA) to constrain the mass accretion rate onto its supermassive black hole. We detected the polarized emission associated with the core at a fractional polarization of 0.73 +/- 0.15%. This low fra...
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Main Authors: | Lo, Wen-Ping, Asada, Keiichi, Matsushita, Satoki, Nakamura, Masanori, Pu, Hung-Yi, Tseng, Chihyin, Akiyama, Kazunori, Algaba, Juan Carlos, Bower, Geoffrey C., Rao, Ramprasad, Koay, Jun Yi, Koch, Patrick M., Koyama, Shoko, Ho, Paul T. P., Inoue, Makoto |
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Format: | Article |
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IOP Publishing Ltd
2021
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Online Access: | http://eprints.um.edu.my/34637/ |
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