======================================================================== G C N E W S * Newsflash * - The Newsletter for Galactic Center Research - gcnews@mpifr-bonn.mpg.de http://www.mpifr-bonn.mpg.de/gcnews ======================================================================== Vol. 11, No. 13 May 4, 2000 Dear subscriber, this is probably the last abstract for Vol. 11 of the newsletter which will be distributed in a few days. So, if you have any announcements to the GC community that should be included in the next issue please send them to us as soon as possible. Recently submitted papers: -------------------------- 1) Sgr A* Polarization: No ADAF, Low Accretion Rate, and Non-Thermal Synchrotron Emission (Agol, ApJL) ------------------------------------------------------------------------ Email : agol@pha.jhu.edu Title : Sgr A* Polarization: No ADAF, Low Accretion Rate, and Non-Thermal Synchrotron Emission Author(s): Eric Agol Institute: Physics and Astronomy Department, Johns Hopkins University, Baltimore, MD 21218; agol@pha.jhu.edu Paper : ApJ Letters, submitted EPrint : astro-ph/0005051 Abstract: The recent detection of polarized radiation from Sgr A* requires a non-thermal electron distribution for the emitting plasma. The Faraday rotation measure must be small, placing strong limits on the density and magnetic field strength. We show that these constraints rule out advection-dominated accretion flow models. We construct a simple two-component model which can reproduce both the radio to mm spectrum and the polarization. This model predicts that the polarization should rise to nearly 100% at shorter wavelengths. The first component, possibly a black-hole powered jet, is compact, low density, and self-absorbed near 1 mm with ordered magnetic field, relativistic Alfven speed, and a non-thermal electron distribution. The second component is poorly constrained, but may be a convection-dominated accretion flow with \dot M 10^-9M_o/yr, in which feedback from accretion onto the black hole suppresses the accretion rate at large radii. The black hole shadow should be detectable with sub-mm VLBI. ------------------------------------------------------------------------ (Older versions of the Newsflash can be found at the gcnews web-page) ======================================================================== Edited by Angela Cotera Heino Falcke (cotera@ipac.caltech.edu) (hfalcke@mpifr-bonn.mpg.de) - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - For Abstract submission please send the (La)Tex file of your paper to gcnews@mpifr-bonn.mpg.de ========================================================================