Recent humps and superhumps observations and an estimation of outburst parameters of the AM CVn star CR Boo
arXiv:2212.07189 · doi:10.1007/s10509-022-04149-z
Abstract
We present our observational results of AM CVn star CR Boo in the UBVR bands. Our observational campaign includes data obtained over 5 nights with the National Astronomical Observatory Rozhen, Belogradchik and the AS Vidojevica telescopes. During the whole time of our observations the brightness of the system varied between in B band. We report the appearance of humps during the period of quiescence and superhumps during the active state of the object, (where the latter are detected in two nights). We obtain the superhumps periodicity for two nights, min. The color during maximum brightness is estimated as and the corresponding temperature is in the range as . We found that CR Boo varies from bluer to redder in the nights with outbursts activity. The star becomes bluer during the times of superhumps.
References in corpus (21)
- Correcting for the Effects of Interstellar Extinction
- Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-Main Sequence Stars
- The Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 microns Using GLIMPSE Data
- Mass Transfer between Double White Dwarfs
- Population synthesis for double white dwarfs. II. Semi-detached systems: AM CVn stars
- Short-period AM CVn systems as optical, X-ray and gravitational wave sources
- Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae
- Early humps in WZ Sge stars
- HST/FGS Parallaxes of AM CVn Stars and Astrophysical Consequences
- V344 Lyrae: A Touchstone SU UMa Cataclysmic Variable in the Kepler Field
- New Method to Estimate Binary Mass Ratios by Using Superhumps
- Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. IV: The Fourth Year (2011-2012)
- Evolution of Close White Dwarf Binaries
- Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. IX: The Ninth Year (2016-2017)
- The Quiescent Spectrum of the AM CVn star CP Eri
- A systematic search for outbursting AM CVn systems with the Zwicky Transient Facility
- New insights into black bodies
- Evidence that short period AM CVn systems are diverse in outburst behaviour
- The outburst of a 60 min AM CVn reveals peculiar color evolution: implications for outbursts in long period double white dwarfs
- Superoutburst of CR Bootis: Estimation of Mass Ratio of a typical AM CVn star by Stage A Superhumps
- Mid-Cycle Observations of CR Boo and Estimation of the System's Parameters