Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4492
Title: One year of monitoring of the 2006 outburst in optical and low radio frequencies
Authors: Anupama, G. C
Keywords: Low Radio Frequencies;RS Ophiuchi;Optical Spectrum
Issue Date: Dec-2008
Publisher: Astronomical Society of the Pacific
Citation: A. Evans, M. F. Bode, T. J. O'Brien, and M. J. Darnley., eds., RS Ophiuchi (2006) and the Recurrent Nova Phenomenon ASP Conference Series, Vol. 401, proceedings of the conference held 12 - 14 June, 2007, at Keele University, Keele, United Kingdom., pp. 251 - 255
Series/Report no.: Astronomical Society of a Pacific Conference Series;Vol. 401
Abstract: The evolution of the optical spectrum of RS Ophiuchi was monitored beginning 1 day since the 2006 outburst discovery to over a year after the outburst. The evolution of the spectrum is found to be similar to previous outbursts. The outburst was also monitored in the low radio frequency region, in the 0.610 GHz, 0.325 GHz and 0.240 GHz bands. The radio observations began ˜ 20 days after the discovery and continued until ˜ 400 days. The outburst was detected, for the first time at frequencies below 1 GHz. The low frequency radio emission is non-thermal and is well-explained by a synchrotron spectrum of index α ˜ -0.8 (S ∝ ν/sup^α) suffering foreground absorption due to the pre-existing, ionized, warm, clumpy red giant wind.
Description: Restricted Access
URI: http://hdl.handle.net/2248/4492
ISSN: 978-1-58381-674-5
???metadata.dc.rights???: © Astronomical Society of the Pacific
???metadata.dc.relation.uri???: http://aspbooks.org/custom/publications/paper/401-0251.html
http://adsabs.harvard.edu/abs/2009ASPC..401..251A
Appears in Collections:IIAP Publications

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