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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Main Authors: Ortiz-León, Gisela N. (Author), Johnson, Michael D. (Author), Blackburn, Lindy (Author), Loinard, Laurent (Author), Reid, Mark J. (Author), Castillo, Edgar (Author), Chael, Andrew A. (Author), Hernández-Gómez, Antonio (Author), Hughes, David H. (Author), León-Tavares, Jonathan (Author), Lu, Ru-Sen (Author), Montaña, Alfredo (Author), Narayanan, Gopal (Author), Rosenfeld, Katherine (Author), Sánchez, David (Author), Schloerb, F. Peter (Author), Shen, Zhi-qiang (Author), Shiokawa, Hotaka (Author), Vertatschitsch, Laura (Author), Doeleman, Sheperd Samuel (Contributor), Fish, Vincent L. (Contributor), SooHoo, Jason G (Contributor)
Other Authors: Haystack Observatory (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2016-10-26T17:58:02Z.
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