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Random forest automated supervised classification of Hipparcos periodic variable stars
We present an evaluation of the performance of an automatedclassification of the Hipparcos periodic variable stars into 26 types.The sub-sample with the most reliable variability types available in theliterature is used to train supervised algorithms to characterize thetype dependencies on a number of attributes. The most useful attributesevaluated with the random forest methodology include, in decreasingorder of importance, the period, the amplitude, the V-I colour index,the absolute magnitude, the residual around the folded light-curvemodel, the magnitude distribution skewness and the amplitude of thesecond harmonic of the Fourier series model relative to that of thefundamental frequency. Random forests and a multi-stage scheme involvingBayesian network and Gaussian mixture methods lead to statisticallyequivalent results. In standard 10-fold cross-validation (CV)experiments, the rate of correct classification is between 90 and 100per cent, depending on the variability type. The main mis-classificationcases, up to a rate of about 10 per cent, arise due to confusion betweenSPB and ACV blue variables and between eclipsing binaries, ellipsoidalvariables and other variability types. Our training set and thepredicted types for the other Hipparcos periodic stars are availableonline.
| Geometrical constraints upon the unipolar model of V407 Vul and RXJ0806.3+1527
V407 Vul and RX J0806.3+1527 are X-ray emitting stars with X-ray lightcurves that are 100 per cent modulated on periods of 569 and 321 s,respectively. These periods and no others are also seen at optical andinfrared wavelengths. These properties have led to the suggestion thatthe periods are the orbital periods of ultracompact pairs of whitedwarfs. There are two main double white dwarf models: the unipolarinductor model analogous to the Jupiter-Io system and the direct impactmodel analogous to Algol. In this paper, we consider geometricalconstraints on the unipolar inductor model, in particular what parametervalues (component masses, orbital inclination and magnetic colatitude)can describe the X-ray and optical light curves. We find that for adipole field on the primary star, the unipolar inductor model fails tomatch the data on V407 Vul for any combination of parameters and canonly match RX J0806.3+1527 if the sparser set of observations of thisstar have been unluckily timed.
| The 74th Special Name-list of Variable Stars
We present the Name-list introducing GCVS names for 3153 variable starsdiscovered by the Hipparcos mission.
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| Takýmyýldýz: | Tilkicik |
| Sað Açýklýk: | 21h06m24.97s |
| Yükselim: | +21°38'06.8" |
| Görünürdeki Parlaklýk: | 9.426 |
| özdevim Sað Açýklýk: | 8.4 |
| özdevim Yükselim: | 0.8 |
| B-T magnitude: | 11.518 |
| V-T magnitude: | 9.599 |
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