F. De Paolis, G. Ingrosso, A. A. Nucita, A. Qadir, A. F. Zakharov
Published 2010-11-06Version 1
The measurement of relativistic effects around the galactic center may allow in the near future to strongly constrain the parameters of the supermassive black hole likely present at the galactic center (Sgr A*). As a by-product of these measurements it would be possible to severely constrain, in addition, also the parameters of the mass-density distributions of both the innermost star cluster and the dark matter clump around the galactic center.
Comments: Accepted for publication on General Relativity and Gravitation, 2010. 11 Pages, 1 Figure
SOFIA/FORCAST Imaging of the Circumnuclear Ring at the Galactic Center
ATCA observations of SiO masers in the Galactic center
A High-Resolution Survey of HI Absorption toward the Central 200 pc of the Galactic Center
![QR code for arXiv:1011.1545 [astro-ph.GA]](http://oss.arxitics.com/images/favicon.svg)