THE INTRINSIC SHAPE OF SAGITTARIUS A* AT 3.5 mm WAVELENGTH

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...

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Bibliographic Details
Main Authors: Ortiz-León, Gisela N., Johnson, Michael D., Blackburn, Lindy, Loinard, Laurent, Reid, Mark J., Castillo, Edgar, Chael, Andrew A., Hernández-Gómez, Antonio, Hughes, David H., León-Tavares, Jonathan, Lu, Ru-Sen, Montaña, Alfredo, Narayanan, Gopal, Rosenfeld, Katherine, Sánchez, David, Schloerb, F. Peter, Shen, Zhi-qiang, Shiokawa, Hotaka, Vertatschitsch, Laura, Doeleman, Sheperd Samuel, Fish, Vincent L., SooHoo, Jason G
Other Authors: Haystack Observatory
Format: Article
Language:en_US
Published: IOP Publishing 2016
Online Access:http://hdl.handle.net/1721.1/105095

Internet

http://hdl.handle.net/1721.1/105095

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