| Detecting Changing Polarization Structures in Sagittarius A* with High Frequency VLBI (2009) | |||||||||
Abstract | |||||||||
| Sagittarius A* is the source of near infrared, X-ray, radio, and (sub)millimeter emission associated with the supermassive black hole at the Galactic Center. In the submillimeter regime, Sgr A* exhibits time-variable linear polarization on timescales corresponding to . Comment: 11 pages, accepted for publication in ApJ | |||||||||
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