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2011CBET.2735....1S - Central Bureau Electronic Telegrams, 2735, 1 (2011/June-0)
Nova Scorpii 2011 = PNV J16551100-3838120.
SEACH J., OKSANEN A., HARLINGTEN C., GUIDO E., SOSTERO G., WILLIAMS P., WAAGEN E., AMORIM A. and MORELL M.
Abstract (from CDS):
Arto Oksanen and Caisey Harlingten report that they obtained images of the suspected nova under partly-cloudy conditions using a 50-cm Dall- Kirkham telescope (+ Apogee Alta CCD camera) located at San Pedro de Atacama, Chile, on June 2.33 UT, yielding preliminary V magnitude 10.4 and position end figures 09s.48, 04".0. Their V-band images spanning a little over an hour show a constant fading of 0.15 mag/hr between June 2.333 and 2.375.
Ernesto Guido and Giovanni Sostero write that they obtained unfiltered CCD images of PNV J16551100-3838120 on June 2.4 UT remotely with the GRAS RCOS 32-cm f/6.3 telescope at Officer, Australia, showing the variable at mag about 9.4 and at R.A. = 16:55:09.46, Decl.= -38:38:04.5 (equinox 2000.0; USNO-B1.0 catalogue reference stars). They have posted an animation showing a comparison between their image and a red Digitized Sky Survey plate from 1995 at website URL http://bit.ly/jK5mMP.
Visual magnitude estimates: June 2.564 UT, 11.2 (Peter Williams, Heathcote, NSW, 15-cm reflector; communicated by E. Waagen, AAVSO); June 2.975 UT, 11.1 [A. Amorim, Florianopolis, Brazil, 0.18-m reflector; magnitude source ASAS-3 chart 73-A00031(d) by Mati Morel].
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