USING MILLIMETER VLBI TO CONSTRAIN RIAF MODELS OF SAGITTARIUS A*

USING MILLIMETER VLBI TO CONSTRAIN RIAF MODELS OF SAGITTARIUS A*

The recent detection of Sagittarius A* at λ = 1.3 mm on a baseline from Hawaii to Arizona demonstrates that millimeter wavelength very long baseline interferometry (VLBI) can now spatially resolve emission from the innermost accretion flow of the Galactic center region. Here, we investigate the abil...

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Bibliographic Details
Main Authors:	Fish, Vincent L., Broderick, Avery E., Loeb, Abraham, Doeleman, Sheperd Samuel
Other Authors:	Haystack Observatory
Format:	Article
Language:	en_US
Published:	IOP Publishing 2015
Online Access:	http://hdl.handle.net/1721.1/96007

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