------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 2979 2014 Feb 08 10.18UT 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 ------------------------------------------------------------------- OUTBURST OF THE RECURRENT NOVA V745 SCO AAVSO Alert Notice 496 carries news that Ron Stubbings, Victoria, Australia noted an outburst of V745 Sco at magnitude 9.0 (visual) on 2014 February 6.694UT. It is located at: RA 17h 55m 22.27s DEC -33 14' 58.5" (2000) Selected observations reported to the AAVSO: Feb 06.694, 9.0 (Stubbings); 06.745, 9.0 (Paul Camilleri, Australia); 06.773, 8.66 V +/-0.06 (S. O'Connor, St. Georges, Bermuda, remotely using iTel17, Siding Spring, NSW, Australia); 7.80903, 10.1 (PEX, A. Pearce, Nedlands, W. Australia); 07.85833, 10.2 (Pearce); 9.483V +/-0.010 (J. Hambsch, Mol, Belgium, remotely at San Pedro de Atacama, Chile); 9.515 V +/-0.009 (Hambsch, remotely); Dr. Bradley Schaefer (Louisiana State University) suggests that fast time-series of this nova may be useful to detect possible flaring activity as was observed during the outburst of U Scorpii in 2010. He suggests that coincident time-series by multiple observers would be most useful for such a study, with a V-filter being preferred. Charts for V745 Sco may be created using the AAVSO Variable Star Plotter (VSP) at http://www.aavso.org/vsp. Previous outbursts occurred in 1937 and 1989. The 1937 outburst was detected in 1958 (in decline at magnitude 11.0 on 1937 May 11.1 UT; outburst had occurred within the previous 19 days) by Lukas Plaut on plates taken by Hendrik van Gent at the Leiden Observatory; the object was announced as Nova Sco 1937 and later assigned the GCVS name V745 Sco. The 1989 outburst was detected on 1989 August 1.55 UT by Mati Morel (MMAT, Thornton, NSW, Australia) at visual magnitude 10.4 and in decline. Congratulations to Rod Stubbings on his detection of the outburst of this difficult pre-dawn recurrent nova! Guy M Hurst