arXiv · astro-ph/9704215
CCD Photometry of SW Ursae Majoris during the 1996 Superoutburst
Abstract
We present CCD R photometry of SW Ursae Majoris - an SUUMa type cataclysmic variable - obtained during its April 1996 superoutburst. The mean value of the superhump period derived from our observations is 0.05818(+/-2) days (83.8 min). The analysis of times of superhump maxima gives clear evidence for the increase of the superhump period with dPsh/dt=0.000089.
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I. Semeniuk, A. Olech, T. Kwast, M. Nalezyty. 1997-04-22. CCD Photometry of SW Ursae Majoris during the 1996 Superoutburst. https://arxiv.org/abs/astro-ph/9704215
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