THE INTRINSIC SHAPE OF SAGITTARIUS A* AT 3.5 mm WAVELENGTH
The radio emission from Sgr A* is thought to be powered by accretion onto a supermassive black hole of ~4 x 10⁶M⊙ at the Galactic Center. At millimeter wavelengths, Very Long Baseline Interferometry (VLBI) observations can directly resolve the bright innermost accretion region of Sgr A*. Motivated b...
Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , , |
---|---|
Weitere Verfasser: | |
Format: | Artikel |
Sprache: | en_US |
Veröffentlicht: |
IOP Publishing
2016
|
Online Zugang: | http://hdl.handle.net/1721.1/105095 |