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.
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Photoelectric observations of Cepheids in UBV(RI)c (Berdnikov, 2008)
This catalog gathers the observation of 894 Cepheids made between 1986to 2004.Observations are listed in alphabetical order of the constellations. Thestandard deviation for every magnitude and color is 0.01mag.This version supersedes the 1997 edition (Cat. )(3 data files).
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Pulkovo compilation of radial velocities for 35495 stars in a common system.
Not Available
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Photometry of Type II Cepheids. III. The Intermediate-Period Stars
We present 741 new photometric observations for 22 Cepheids with periodsbetween 3 and 8 days. Many of the stars are probable type II Cepheids,but we have included some type I Cepheids for comparison. The shapes andstability of the shapes of the light curves, the stability of theperiods, and the scatter of individual data points are discussed.Although none of these proves to be a reliable discriminator betweentype I and type II Cepheids, they do permit the identification ofseveral unusual stars.
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The Spectra of Type II Cepheids. II. The Hα Line in Intermediate-Period Stars
We present 98 Hα profiles for 21 pulsating variable stars withperiods from 3 to 8 days. The strength, depth, and shape of Hαvary throughout the cycles of the stars in a way consistent with thetemperature changes. Otherwise, they are quite uniform among all thestars, with a single exception. In FM Del, Hα is weaker and has asmaller central depth than in the other stars. This and the wavelengthshifts of the core are attributed to incipient emission. Thedifferential velocity of Hα relative to the metal lines is lessthan 25 km s-1 for all the stars except QY Cyg, FM Del, andEF Tau. We suggest that this indicates that only these stars are type IICepheids despite the large distances of some of the others from theGalactic plane.Based in part on observations obtained with the Apache Point Observatory3.5 m telescope, which is owned and operated by the AstrophysicalResearch Consortium.
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Stars with the Largest Hipparcos Photometric Amplitudes
A list of the 2027 stars that have the largest photometric amplitudes inHipparcos Photometry shows that most variable stars are all Miras. Thepercentage of variable types change as a function of amplitude. Thiscompilation should also be of value to photometrists looking forrelatively unstudied, but large amplitude stars.
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A catalog of Cepheid radial velocities measured in 1995-1998 with the correlation spectrometer
We present a catalog of 2444 original radial-velocity measurements for108 Cepheids based on the 1995-1998 observations with the correlationspectrometer. Detailed radial-velocity curves are given for 12 Cepheidsfor the first time.
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Spectroscopic survey of field Type II Cepheids
A sample of relatively bright, short- and intermediate-period (P=1-10d)Type II Cepheids in the Galactic field have been observedspectroscopically with an intermediate-resolution(lambda/Deltalambda=11000) spectrograph. The wavelength region was6500-6700A, including the Hα line and some photospheric ironlines. The signal-to-noise ratio (S/N) was usually between 50 and 100,depending on weather conditions and the brightness of target stars.Radial velocities were determined by cross-correlating the Cepheidspectra with those of selected IAU velocity standard stars having F-Gspectral types. The internal error of the velocity determination processwas calculated to be about 1 km s^-1. Hα emission and strong linesplitting were observed in BL Her during the expansion phase, but nosimilar phenomenon was detected in any other stars in this programme,except for AU Peg which has an unusual Hα line showing a PCygni-like profile. The velocity curve agrees well with recent CORAVELmeasurements. The velocity gradients in Cepheid atmospheres are studiedusing the Hα minus metallic velocities. Similar data are collectedfrom the literature. It seems that having large velocity differences(v_Hα-v_metal>40 km s^-1) is a characteristic feature of thevery short-period (P<1.5d) and longer period (P>10d) Cepheids.Between these period regions the Cepheid atmospheres exhibit smallervelocity differences. Most of the Type II Cepheids observed in thepresent study fall into this latter category. There might be a tendencyfor classical Cepheids of intermediate period to have larger maximumvelocity differences.
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The radii of 62 classical Cepheids
Based on dense series of photoelectric observations and on ourradial-velocity measurements, we calculated the radii of 62 northernCepheids by Balona's method. We derived the following period-radiusrelation: log R = 1.23(+/-0.03) + 0.62(+/-0.03) log P. Our detailedanalysis shows that the distance scale for Cepheids cannot be refinedusing their radii by an independent method which is unrelated to thedistances to young open clusters because of the random and systematicerrors of the Baade-Wesselink technique.
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Spectroscopic binary orbits from ultraviolet radial velocities. Paper 22: HD 48099
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A catalog of Cepheid radial velocities measured in 1992-1995 with a correlation spectrometer
Not Available
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Faint Cepheid Studies. I. Comparison With Existing Data Sets
UBVRI data on 36 short-period (P < 5 days) cepheids is given. Theobserving techniques and reduction procedures are described. Aconsistent set of finding charts, a set of standard stars for eachcepheid, and improved coordinates are also presented.
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Mean radial velocities and binarity of cepheids from the 1987-1995 measurements
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Rotation curve of the system of classical Cepheids and the distance to the galactic center
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Classical Cepheids - Their distances and space distribution
A simplified method of calculating classical Cepheid distances isproposed. It is based on photometric data, without the use of thereddenings. By means of results obtained in this way the followingproblems are discussed: Cepheid double and more numerous aggregates andproperties of the cluster and association Cepheid.
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The catalogue of light curves parameters, distances and space coordinates of classical Cepheids.
Not Available
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A catalogue of field Type II Cepheids
A catalogue of field Type II Cepheids is presented. The primary listconsists of 152 Cepheids sufficiently far from the galactic plane to bevery probably Type II stars. A second list contains 56 additional starsthat are likely, but less certain, Type II Cepheids, including bothstars estimated to be at large distances from the galactic plane butwith uncertain distances and stars close to the galactic plane believedto be Type II for independent reasons.
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The Catalogue of Distances and Light Absorption for Cepheids
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The light curve parameters of photoelectrically observed galactic Cepheids
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1971A&AS....4..265S&db_key=AST
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The Normal Color Indices and Color Excesses of Long-Period Cepheids.
Not Available
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Faint Cepheids in Cygnus and Monoceros
Abstract image available at:http://adsabs.harvard.edu/abs/1969ApJ...156..617E
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Le type de population des céphéides galactiques; critères de distinction des types et catalogue
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Studies on Galactic Cepheids System. I. Absorption of Cepheids with known radial velocities and a nomogram for the computation of the galactocentric distance
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A search for Cepheids in galactic clusters.
Abstract image available at:http://adsabs.harvard.edu/abs/1957ApJ...126..323V
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The value of the Oort A parameter derived from radial velocities of Cepheid variable stars.
Abstract image available at:http://adsabs.harvard.edu/abs/1955AJ.....60..202W
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Benennung von veränderlichen Sternen
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