Received: from relay.micronet.it (root@mother.micronet.it [194.20.45.1]) by ceres.kusastro.kyoto-u.ac.jp (8.8.8+3.0Wbeta13/3.6W98052214) with ESMTP id GAA16504 for <vsnet-chat@kusastro.kyoto-u.ac.jp>; Sat, 26 Sep 1998 06:10:12 +0900 (JST) Received: from line27.micronet.it (line27.micronet.it [194.20.45.187]) by relay.micronet.it (8.8.5/8.8.5/NOSPAM) with SMTP id XAA20258; Fri, 25 Sep 1998 23:09:56 +0200 Date: Fri, 25 Sep 1998 23:09:56 +0200 Message-ID: <10001330@hoge.baba.hajime.jp> X-Sender: peste@micronet.it X-Mailer: Windows Eudora Version 1.4.4 Mime-Version: 1.0 Content-Type: text/plain; charset="us-ascii" To: isn_chat@mbox.queen.it From: peste@micronet.it (Stefano Pesci) Cc: vsnet-chat@kusastro.kyoto-u.ac.jp Precedence: list X-Distribute: distribute [version 2.1 (Alpha) patchlevel=24] X-Sequence: vsnet-chat 0 Subject: [vsnet-chat 0] Re: SN 1998eb in NGC 1961 Errors-To: owner-vsnet-chat@kusastro.kyoto-u.ac.jp Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp Dear Friends, according to my sources NGC 1961 has a distance modulus in the 33.3-34 range. If the sn is type Ia then its apparent magnitude at maximun would have been in the 15.0 15.5 range, easily detectable visually, within the time frame indicated by IAUC 7018. I suspect though that the supernova is quite absorbed by the host galaxy and may have not reached that brightness. Good observing. _________________________________________________ Stefano Pesci, peste@micronet.it, Milan, ITALY _________________________________________________ International Supernova Network: http://vsnet.supernovae.org/isn.htm _________________________________________________