Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.2 9/18/84; site utastro.UUCP Path: utzoo!linus!philabs!cmcl2!seismo!ut-sally!utastro!ethan From: ethan@utastro.UUCP (Ethan Vishniac) Newsgroups: net.astro Subject: Re: StarDate: October 12 The Halo of the Milky Way Message-ID: <50@utastro.UUCP> Date: Tue, 15-Oct-85 18:35:03 EDT Article-I.D.: utastro.50 Posted: Tue Oct 15 18:35:03 1985 Date-Received: Thu, 17-Oct-85 20:21:07 EDT References: <38@utastro.UUCP> <2140@brl-tgr.ARPA> Organization: U. Texas, Astronomy, Austin, TX Lines: 25 > > Or is this a currently-debated topic in astronomy, > and things are not as clearly agreed-upon as the impression I got from > the Disney book leads me to think? > > Will Bingo. Actually, the massive halo need only weigh about as much as the visible galaxy to stabilize the disk. Virial theorem measurements of galaxy masses have led people to propose much larger halo masses. There is some controversy over exactly how massive the halo needs to be to explain these results. If the halo is very massive then it is not composed of stars. This leaves open the possibility that it is composed of black holes or white dwarfs. It is not likely to be dust or monotomic gas. Could be molecular hydrogen but its formation would be a mystery. Could be Jupiters (i.e. generic gas giant objects). Could be Weakly Interacting Massive Particles (acronym is widely used). -- "Superior firepower is an Ethan Vishniac important asset when {charm,ut-sally,ut-ngp,noao}!utastro!ethan entering into ethan@astro.UTEXAS.EDU negotiations" Department of Astronomy University of Texas