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1.3 mm Wavelength VLBI of Sagittarius A*: Detection of Time-Variable Emission on Event Horizon Scales
Vincent L. Fish, Sheperd S. Doeleman, Christopher Beaudoin +27
Sagittarius A*, the ~4 x 10^6 solar mass black hole candidate at the Galactic Center, can be studied on Schwarzschild radius scales with (sub)millimeter wavelength Very Long Baseli…
The High-Density Ionized Gas in the Central Parsec of the Galaxy
Jun-Hui Zhao, Ray Blundell, James M. Moran +3
We report a study of the H30 line emission at 1.3 mm from the region around Sgr A* made with the Submillimeter Array at a resolution of 2\arcsec\ over a field of 60\arcsec\ (2 p…
The High-Density Ionized Gas in the Central Parsecs of the Galaxy
Jun-Hui Zhao, Ray Blundell, James M. Moran +3
We report the results from observations of H30 line emission in Sgr A West with the Submillimeter Array at a resolution of 2\arcsec and a field of view of about 40\arcsec. The H…