ﻻ يوجد ملخص باللغة العربية
A recent analysis of high precision photometry obtained using the Kepler spacecraft has revealed two surprising discoveries: (1) over 860 main sequence A-type stars -- approximately 40% of those identified in the Kepler field -- exhibit periodic variability that may be attributable to rotational modulation by spots and (2) many of their light curves indicate the presence of a mysterious and characteristic power spectral feature. We have been carrying out an ongoing analysis designed to expand upon these discoveries and to provide a possible explanation for the unusual power spectral features. In the following, we will put these recent discoveries into context as well as discuss the preliminary findings yielded by our analysis of the Kepler light curves.
Recent re-determination of stellar atmospheric parameters for a sample of stars observed during the {it Kepler} mission allowed to enlarge the number of {it Kepler} B-type stars. We present the detailed frequency analysis for all these objects. All s
The analysis of the light curves of 48 B-type stars observed by Kepler is presented. Among these are 15 pulsating stars, all of which show low frequencies characteristic of SPB stars. Seven of these stars also show a few weak, isolated high frequenci
The Kepler spacecraft is providing photometric time series with micro-magnitude precision for thousands of variable stars. The continuous time-series of unprecedented time span open up opportunities to study the pulsational variability in much more d
The Kepler spacecraft is providing time series of photometric data with micromagnitude precision for hundreds of A-F type stars. We present a first general characterization of the pulsational behaviour of A-F type stars as observed in the Kepler ligh
The advent of new time domain surveys and the imminent increase in astronomical data expose the shortcomings in traditional time series analysis (such as power spectra analysis) in characterising the abundantly varied, complex and stochastic light cu