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TESS light curves of cataclysmic variables -- III -- More superhump systems among old novae and novalike variables
Albert Bruch
Continuing previous work on the identification and characterization of periodic and non-periodic variations in long and almost uninterrupted high cadence light curves of cataclysmi…
Orbital Periods and Waveforms of Dwarf Novae Observed by Kepler
Albert Bruch
Kepler high cadence data are used to measure the orbital periods and to determine the orbital waveforms of five dwarf novae. A significant improvement of the period of V1504 Cyg is…
A comparative study of the strength of flickering in cataclysmic variables
Albert Bruch
Flickering is a universal phenomenon in accreting astronomical systems which still defies detailed physical understanding. It is particularly evident in cataclysmic variables (CVs)…
Miscellaneous photometric variations in cataclysmic variables: V455 And, SS Cyg, AQ Men, LQ Peg, RW Tri and UX UMa
Albert Bruch
Cataclysmic variables are among the photometrically most unstable stars in the zoo of stellar objects, exhibiting light variations on all time-scales between millennia and seconds.…
TT Arietis: 40 years of photometry
Albert Bruch
In an effort to characterize variations on the time scale of hours and smaller during the high and low states of the novalike variable TT Ari, light curves taken over the course of…
UU Aqr - No superhumps but variations on the time scale of days
Albert Bruch
Recently, brightness variations occurring on twice the accretion disk precession period in the old nova and permanent superhump system V603 Aql have been observed by Bruch & Cook (…