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: | , , , , , , , , , , , , , , |
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Format: | Article |
Published: |
IOP Publishing Ltd
2021
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Subjects: | |
Online Access: | http://eprints.um.edu.my/34637/ |
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