CCD Photometry of SW Ursae Majoris during the 1996 Superoutburst

Details CCD Photometry of SW Ursae Majoris during the 1996 Superoutburst CCD Photometry of SW Ursae Majoris during the 1996 Superoutburst

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998pasj...50..297n&link_type=abstract

Publications of the Astronomical Society of Japan, v.50, p.297-302.

Astronomy and Astrophysics

Astronomy

26

Accretion, Accretion Disks, Stars: Cataclysmic, Stars: Dwarf Novae, Stars: Individual (Sw Ursae Majoris)

Scientific paper

Differential CCD photometry of the 1996 April superoutburst of SW UMa was performed both at the Nicholas Copernicus Observatory and at the Ouda Station, Kyoto University. Although superhumps with a period of 0.05818 (+/- 0.00002) d and possible small-amplitude quasi periodic oscillations (QPOs) were detected, we failed to find the so-called super-QPOs. SW UMa has been proved to be the fourth SU UMa-type dwarf nova, following AL Com, V1028 Cyg, and HV Vir, in which an analysis of the superhump maxima timings revealed an increase in the superhump period.

Affiliated with

Also associated with

No associations

Rating

CCD Photometry of SW Ursae Majoris during the 1996 Superoutburst does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with CCD Photometry of SW Ursae Majoris during the 1996 Superoutburst, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CCD Photometry of SW Ursae Majoris during the 1996 Superoutburst will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1744083