Hallo, attached you find the circular we submitted to IAU on May 1st - I do not know why it has not appeared yet. Marina Orio --------------------------------------------------------------------- Marina Orio: In Wisconsin: Astronomy Dept., 475 N. Charter Str., 53706 Madison WI Phone +1-608-262-9387 Fax +1-608-263-0800 orio@cow.physics.wisc.edu In Italy: National Institute for Astrophysics (INAF) Osservatorio Astronomico di Torino, Strada Osservatorio 20, Pino Torinese (TO), I-10025 Italy Tel +39-011-8101910 Fax +39-011-8101930 orio@to.astro.it --------------------------------------------------------------------
From MAILER-DAEMON Sun May 5 09:58:22 2002 Date: Sun, 5 May 2002 09:58:22 -0500 (CDT) From: Mail System Internal Data <MAILER-DAEMON@cow.physics.wisc.edu> Subject: DON'T DELETE THIS MESSAGE -- FOLDER INTERNAL DATA X-IMAP: 1020610702 0000000000 Status: RO This text is part of the internal format of your mail folder, and is not a real message. It is created automatically by the mail system software. If deleted, important folder data will be lost, and it will be re-created with the data reset to initial values. From orio@cow.physics.wisc.edu Wed May 1 15:14:52 2002 -0500 Status: R X-Status: X-Keywords: Date: Wed, 1 May 2002 15:14:51 -0500 (CDT) From: Marina Orio <orio@cow.physics.wisc.edu> To: cbat@cfa.harvard.edu Subject: Re: Discovery to submit Message-ID: <Pine.OSF.4.03.10205011436170.30713-100000@cow.physics.wisc.edu> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII Hallo, We would like to report the following discovery on a IAU Circular: "Images of the "light echo" around V838 Mon (IAUC 7859) taken with the WIYN 3.5m telescope (0".141/pixel) in the R band and with an H(alpha) narrow filter on April 19 2002, in V band and with an [OIII] narrow filter on April 21 2002. show a filled shell, approximately circular, and not limb brightened, with a 35 arcsec diameter on both nights. (See http://cow.physics.wisc.edu/~orio/v838monb.html). The contour of the shell is irregular, with a broad structure in the shape of an arc and clumps, but no small scale structure. There is more structure in V than in R. Lack of conspicuous H(alpha) and [OIII] line emission confirms that it is a reflection rather than a ionization nebula. An image obtained on April 30 at the WIYN 90cm telescope (scale 0".60 arcsec/pixel) in R band still shows a 35 arcsec diameter, so the outer edge of the reflecting material was reached before April 22." M. Orio (INAF-Torino and Univ. Wisconsin), D. Harbeck (Max Planck Inst. Astron., Heidelberg) and J. Gallagher and C. Woodward (Univ. Wisconsin). --------------------------------------------------------------------- Marina Orio: In Wisconsin: Astronomy Dept., 475 N. Charter Str., 53706 Madison WI Phone +1-608-262-9387 Fax +1-608-263-0800 orio@cow.physics.wisc.edu In Italy: National Institute for Astrophysics (INAF) Osservatorio Astronomico di Torino, Strada Osservatorio 20, Pino Torinese (TO), I-10025 Italy Tel +39-011-8101910 Fax +39-011-8101930 orio@to.astro.it --------------------------------------------------------------------