------------------------------------------------------------------------ Alexander05_physreps.tex invited review, Physics Reports,2005, in press X-Enigmail-Version: 0.84.0.0 X-Enigmail-Supports: pgp-inline, pgp-mime Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-ESAFE-STATUS: Mail clean X-ESAFE-DETAILS: Clean X-MailScanner-Information: Please contact postmaster@aoc.nrao.edu for more information X-MailScanner: Found to be clean X-MailScanner-SpamCheck: not spam, SpamAssassin (score=-0.1, required 5, USER_AGENT 0.00, X_ACCEPT_LANG -0.10) %astro-ph/0508106 \documentclass[12pt,twoside,english,fleqn,twoside,executivepaper]{article} \title{Stellar Processes Near the Massive Black Hole in the Galactic Center} \author{Tal Alexander} \affil{Faculty of Physics, The Weizmann Institute of Science, PO Box 26, Rehovot 76100, Israel} \begin{abstract} A massive black hole resides in the center of most, perhaps all galaxies. The one in the center of our home galaxy, the Milky Way, provides a uniquely accessible laboratory for studying in detail the connections and interactions between a massive black hole and the stellar system in which it grows; for investigating the effects of extreme density, velocity and tidal fields on stars; and for using stars to probe the central dark mass and to probe post-Newtonian gravity in the weak- and strong-field limits. Recent results, open questions and future prospects are reviewed in the wider context of the theoretical framework and physical processes that underlie them. \end{abstract} -- Tal Alexander Faculty of Physics, Weizmann Institute of Science PO Box 26, Rehovot 76100, Israel Phone ++972-8-934-4483, Fax ++972-8-934-4477 Email tal.alexander@weizmann.ac.il