Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.2 9/18/84; site watdcsu.UUCP Path: utzoo!watmath!watdcsu!herbie From: herbie@watdcsu.UUCP (Herb Chong [DCS]) Newsgroups: net.physics Subject: Re: Color of Neutron Stars. Message-ID: <1218@watdcsu.UUCP> Date: Sat, 6-Apr-85 18:25:20 EST Article-I.D.: watdcsu.1218 Posted: Sat Apr 6 18:25:20 1985 Date-Received: Sun, 7-Apr-85 05:30:26 EST References: <1523@decwrl.UUCP> Reply-To: herbie@watdcsu.UUCP (Herb Chong [DCS]) Organization: U of Waterloo Lines: 20 Summary: In article <1523@decwrl.UUCP> cooper@pbsvax.DEC (Topher Cooper) writes: >It was speculated that that matter would be mostly or wholly >iron (the trough in the curve of binding energy). It would >be expected that the "typical" neutron star would have a >very intense magnetic field, a result of compression of the >"ancestral" stars ordinary magnetic field. This field would >be expected to be intense enough to cause the iron from the >surface to form into "hairs" similar to the lines of iron >filings formed with a bar magnet. > <..> > Topher Cooper would this not then imply (because of the extremely rough surface) that the star would radiate as an almost perfect black body? an outside observer would see (ignoring many things such as atmosphere) a redshifted black body at the temprature of the surface. Herb Chong... I'm user-friendly -- I don't byte, I nybble....