M96に明るい超新星らしき天体が発見された模様です。発見者はイタリアの Mirko Villiです。まだIAUCは発行されていませんが、近傍銀河で初期観測が 大変貴重であることから、Brian Skiffとの相談の上vsnet-alertで広報するこ とにしました。現在増光中。もしIa型であれば10等台も期待できます。 この辺で山岡さんにバトンタッチかな? From owner-vsnet-alert@kusastro.kyoto-u.ac.jp Sun May 10 16:39 JST 1998 Date: Sun, 10 May 1998 00:36:36 -0700 From: bas@lowell.Lowell.Edu (Brian Skiff) Subject: [vsnet-alert 1755] Supernova in NGC 3368 = Messier 96 Mirko Villi in Italy has found (on May 9.9 UT) an apparent supernova in the bright galaxy Messier 96. He reports that it is located about 50 arcsec north of the center of the galaxy and about mag. 13.5. I have made a visual confirmation of this object using the Lowell 53cm telescope at May 10.33 UT. The position estimate seems to be correct based on offsets using the telescope's photometer diaphragms. If anything, the star has become quite a bit brighter in the intervening 6-8 hours, and must be at least mag. 12.5 if not 12.0---because of the Full Moonlight and high aerosols scattering it, I could see nothing in the field except the galaxy nucleus and the new star. There is no asteroid here in either the Minor Planet Center's search widget or from our local asteroid database. The object does not appear on various images of the galaxy (Vickers, Hubble/Carnegie, POSS, Wray color atlas, etc.). \Brian 次は周辺比較星情報です。 From owner-vsnet-alert@kusastro.kyoto-u.ac.jp Sun May 10 17:11 JST 1998 Date: Sun, 10 May 1998 01:08:28 -0700 From: bas@lowell.Lowell.Edu (Brian Skiff) Subject: [vsnet-alert 1756] T&B sequence around Messier 96 As far as I know, there is no published photometric sequence around M96. On the relevant chart from the Thompson & Bryan "Supernova Search Charts" are shown V magnitudes evidently from several professional observers. Below are the positions and IDs for these stars (except a faint star very close to the galaxy). The name indicates the magnitude rounded to 0.1, e.g. "114" means V = 11.4. ID RA (2000) Dec GSC 114 10 46 23.9 +11 56 54 0849-0685 126 10 46 21.7 +11 44 29 0849-0703 131 10 46 32.7 +11 50 55 0849-0841 135 10 46 10.4 +11 42 50 0849-0887 143 10 46 52.9 +11 43 22 0849-0306 149 10 46 52.9 +11 52 42 0849-0206 150 10 46 32.7 +11 52 06 0849-0931 T&B give the sources for this data as Peter Birch et al. (Perth Observatory, Western Australia), Bill Liller and Gonzalo Alcaino (CTIO?), and Marion Frueh (probably McDonald Observatory). Since I complain that the IAUC's don't give a precise position for the host galaxies of supernovae, the center of M96 is at: 10 46 45.6 +11 49 18 (2000), according to NED, which cites 1996 ApJS 107, 215, and claims an accuracy of +/- 5 arcsec. \Brian