The Galactic Center

5Citations
Citations of this article
11Readers
Mendeley users who have this article in their library.

Abstract

In the past decade high resolution measurements in the infrared employing adaptive optics imaging on 10m telescopes have allowed determining the three dimensional orbits stars within ten light hours of the compact radio source at the center of the Milky Way. These observations show the presence of a three million solar mass black hole in Sagittarius A* beyond any reasonable doubt. The Galactic Center thus constitutes the best astrophysical evidence for the existence of black holes which have long been postulated, and is also an ideal lab for studying the physics in the vicinity of such an object. Remarkably, young massive stars are present there and probably have formed in the innermost stellar cusp. Variable infrared and X-ray emission from Sagittarius A* are a new probe of the physical processes and space-time curvature just outside the event horizon. © 2007 International Astronomical Union.

Author supplied keywords

Cite

CITATION STYLE

APA

Genzel, R., & Karas, V. (2006). The Galactic Center. In Proceedings of the International Astronomical Union (Vol. 2, pp. 173–180). https://doi.org/10.1017/S1743921307004929

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free