VLBI Studies of Sgr A*

Details VLBI Studies of Sgr A* VLBI Studies of Sgr A*

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005jkas...38..261s&link_type=abstract

Journal of the Korean Astronomical Society, vol. 38, no. 2, pp. 261-266

Astronomy and Astrophysics

Astronomy

2

Galaxy: Center, Galaxies: Individual (Sagittarius A*), Techniques: Interferometric

Scientific paper

This paper reviews the progress in the VLBI (Very Long Baseline Interferometry) studies of Sgr A*, the best known supermassive black hole candidates with a dark mass concentration of 4×10^6 M&sun; at the center of the Milky Way. The emphasis is on the importance of the millimeter and sub-millimeter VLBI observations in the detection of Sgr A*'s intrinsic structure and search for the structural variation.

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