------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 2505 2008 Dec 09 16.55UT Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise, Basingstoke, Hants, RG22 4PP,England.Telephone/FAX(01256)471074Int:+441256471074 INTERNET: GUY@TAHQ.DEMON.CO.UK Backup: gmh@wdcc1.bnsc.rl.ac.uk WORLD WIDE WEB http://www.theastronomer.org ------------------------------------------------------------------- M31N2008-11b - A DWARF NOVA IN OUR GALAXY? Koichi Itagaki, Japan reports on CBET 1588 discovery of a possible bright apparent nova in M31 on unfiltered CCD survey frames taken on 2008 Nov. 26.498 UT using a 0.60-m f/5.7 reflector. The new object is located at: RA 00h 42m 26.50s DEC +42 15' 36.7"(2000). Nothing is visible at this position on the Digitised Sky Survey (DSS) to limiting magnitude 21. Available magnitudes from Itagaki for the apparent nova: 2007 Oct. 13.635, [20.5; 2008 Nov. 26.498, 19.0; 26.538, 18.8; 26.548, 18.8; 26.561, 18.6; 26.564,18.5; 26.565, 18.4; 26.581, 18.2; 28.642, 14.5; 28.643, 14.5; 28.645, 14.6;28.651, 14.5; 28.663, 14.6; 28.714, 14.7; 28.739, 14.9. Nakano forwards the following position end figures measured by K. Kadota: 26s.51, 36".7 (mag 14.7 on Nov.28.694). Kadota adds that nothing is visible on a red DSS image from 1989. M. M. Kasliwal, R. Quimby, S. R. Kulkarni (Caltech) report on ATEL No. 1867 that they observed M31N2008-11b with the Double Beam Spectrograph on the Palomar Hale 5-m telescope on UT Dec 4.221. This spectrum has a steep blue continuum, very narrow emission in H-alpha and broad absorption in H-beta through at least H-eta. Further, there is a faint blue counterpart in SDSS DR Supplement g-band imaging (g=22.8, r > 23.3). Given the reported peak magnitude of 14.5 (CBET#1588), this outburst had an amplitude of >8 mag. We suggest that this optical transient is an SU-UMa-like superoutburst in our own galaxy similar to HS2219+1824 (Rodriguez-Gil et al 2005). SUPERNOVA 2008hj IN MCG -02-1-14 Discovery by the Puckett Observatory Supernova Search of a possible supernova (CBET 1579): SN 2008 UT R.A. (2000.0) Decl. Mag. Offset 2008hj Nov 20.14 00 04 01.91 -11 10 07.5 17.2 5.3"E,19.9"N SUPERNOVA 2008hk IN ANONYMOUS GALAXY Discovery by the Catalina Real-time Transient Survey of a possible supernova (CBET 1581): SN 2008 UT R.A. (2000.0) Decl. Mag. Offset 2008hk Nov 6.49 09 12 43.63 +09 55 47.9 16.7 0.1"E, 0.5"N R. Chornock et. al., University of California, Berkeley, report that spectra of Nov. 23 UT using the Kast spectrograph on the Lick 3-m telescope, reveal that it is a type-Ia supernova with a best-fit age of 16 +/- 3 days after maximum light. V358 LYRAE Further to the reported outburst on E2501, Gary Poyner, Birmingham, England reports the object has re-brightened: Dec 5.874 19.55C 7.878 17.28C Bradford Robotic Telescope Guy M Hurst