Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10 5/3/83; site noao.UUCP Path: utzoo!watmath!clyde!burl!ulysses!allegra!princeton!astrovax!noao!allan From: allan@noao.UUCP Newsgroups: net.astro.expert Subject: Re: neutron stars, black holes, etc. (less long) Message-ID: <342@noao.UUCP> Date: Tue, 22-May-84 12:08:48 EDT Article-I.D.: noao.342 Posted: Tue May 22 12:08:48 1984 Date-Received: Wed, 23-May-84 09:05:26 EDT References: <303@utastro.UUCP> Organization: Natl. Optical Astronomy Obs. Tucson AZ USA Lines: 10 I stand corrected about rotation being the only way of producing a stable frequency of pulsation. However, the difference between pulsars and the ZZ Ceti stars is that pulsars give strong radio pulses, not optical pulses. While I agree that optical pulses can be produced by non rotational methods, radio pulses are much more difficult. Peter (theories to go) Allan Kitt Peak National Observatory Tucson, Az