------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 2598 2009 Nov 26 10.22UT 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 ------------------------------------------------------------------- POSSIBLE NOVA IN ERIDANUS K. Itagaki of Yamagata, Japan has reported on CBET 2050 his discovery of a possible magnitude 8.1 nova on 2009 Nov. 25.536 UT with his 0.21-m patrol system. A confirming image by him on Nov. 25.545 with a 0.60-m reflector shows the object at: RA 04h 47m 54.21s DEC-10 10' 43.1"(2000). Itagaki notes that there is a faint (mag about 15) object near this position on his archival patrol images. Yamaoka suggests that it might be the brightening of a mag 15 blue star that is contained in many catalogues (USNO-B1.0 position end figures 54.19s, 42.9"), though the suggested amplitude of seven magnitudes is perhaps rather large for a dwarf nova but small for a rapid classical nova. Yamaoka adds that the ASAS-3 system (Pojmanski 2002, Acta. Astron. 52, 397) also detected this object at the following V magnitudes: 2009 Nov. 10.236UT, [14.0:; 19.241, 7.34; 22.179, 7.98; 24.269, 8.12. The AAVSO advise on special notice 181 that finder charts for this object may be plotted using VSP by entering the coordinates into the form at the URL http://www.aavso.org/observing/charts/vsp/. An e-mail was received at TAHQ today at 10h24mUT during preparation of this circular from Ernesto Guido and Giovanni Sostero. They advise that using the 0.25-m, f/3,4 reflector + CCD, from GRAS Observatory (near Mayhill, NM) they confirmed the presence of the optical transient on Nov 26.36UT at magnitude 8.2 based on using an unfiltered CCD. They derived the following position (UCAC2 Catalogue reference stars) RA 04h 47m 54.12s DEC -10 10' 43.1" (2000) They add that a comparison with a DSS red plate (limiting magnitude about 20), obtained on 1990, Nov. 23, shows the proximity of a mag 15 star to the position of the possible nova in Eri. Guy M Hurst