------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 2943 2013 Aug 16 14.12UT 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 ------------------------------------------------------------------- NOVA DELPHINI 2013 Further to the note on E-Circular 2942, recent observations suggest the object is still brightening since discovery. Recent visual estimates: 2013 Aug 15.00UT, 6.1 (Bjorn Granslo, clouds, 10x50B) 2013 Aug 15.48UT, 5.6 (Paul Camilleri, 20x80B) 2013 Aug 15.91UT, 5.4 (Guy Hurst, 15x80B thin cloud) The AAVSO 15 deg chart can be obtained from this link: http://www.aavso.org/tmp3/d25315.png There was also a chart included in TA Early Warning Circular 198 issued on August 15, a copy of which can be e-mailed on request to the editor. T. Tomov et. al, institute of Astronomy and NAO, Sofia, Bulgaria report on The Astronomer's Telegram 5288 optical BV photometry and spectroscopy obtained between 2013 August 14.88UT-15.08UT. Using a 0.60-m Cassegrain telescope at the Nicolaus Copernicus University Observatory (Torun, Poland) they estimated the V brightness of the nova to be 6.31+/-0.02 mag and 6.18+/-0.03 mag on Aug. 14.94 UT and Aug. 15.02 UT respectively. The (B-V) colour of the nova was 0.19 and 0.21 mag respectively, showing a reddening of ~0.02 mag in about two hours. Spectral observations were performed in the 4400-7000 AA range using the echelle spectrograph (R~11000) attached to the 60/90 cm Schmidt-Cassegrain telescope (Torun, Poland) and in regions covering ~200 A around Halpha, Hbeta and NaI (R~16000) using the Coude spectrograph of the 2 m RCC telescope at the Rozhen Observatory (Rozhen, Bulgaria). The strongest features of the spectrum are the Balmer lines demonstrating P Cyg profiles. The Halpha emission shows a flat top. The radial velocity measured at the minima of the P Cyg absorptions is about -1600 km/sec. SUPERNOVA 2013eh (THU-NAOC TRANSIENT SURVEY) 2013eh Jly 19.19 16 16 09.19 +38 32 53.0 16.6 4.7"W 8.0"N Dave Balam, Dominion Astrophysical Observatory, National Research Council of Canada et. al., report a spectrum of July 21 shows a type-Ia supernova one week before maximum. SUPERNOVA 2013ei IN NGC 7068 (ASAS-SN) 2013ei Jun 26.47 21 26 31.93 +12 10 49.4 16.0 14 "W 6 "S Villanueva: spectrum June 29 type-Ia supernova around maximum. SUPERNOVA 2013ek IN NGC 6984 (STUART PARKER) 2013ek Jly 24.45 20 57 53.90 -51 52 24.5 16.9R 1 "W 10 "S Parker noted the closeness of this variable to the position of SN 2012im. D. Milisavljevic: spectrum July 25 young type-Ib/c supernova SUPERNOVA 2013el IN NGC 1285 (STUART PARKER) 2013el Jly 11.79 03 17 52.45 -07 18 02.1 15.5R 14 "W 10 "S S. Valenti: spectrum July 13 type-Ib Guy M Hurst