CCD Photometry of SW Ursae Majoris during the 1996 Superoutburst

Simple item page
dc.creatorSemeniuk, I.
dc.creatorOlech, A.
dc.creatorKwast, T.
dc.creatorNalezyty, M.
dc.date1997-04-22
dc.date.accessioned2026-07-25T20:22:17Z
dc.descriptionWe 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.
dc.descriptionaccepted in publication in Acta Astronomica (Vol. 47, p. 201), 6 pages, LaTeX file with 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9704215
dc.identifierhttp://arxiv.org/abs/astro-ph/9704215
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/70628
dc.subjectAstrophysics
dc.titleCCD Photometry of SW Ursae Majoris during the 1996 Superoutburst
dc.typetext

Files

Collections

Artificial intelligence