A catalogue of eclipsing variables A new catalogue of 6330 eclipsing variable stars is presented. Thecatalogue was developed from the General Catalogue of Variable Stars(GCVS) and its textual remarks by including recently publishedinformation about classification of 843 systems and making correspondingcorrections of GCVS data. The catalogue1 represents thelargest list of eclipsing binaries classified from observations.
|
Updated Elements for Southern Eclipsing Binaries Analysis of ASAS-3 data for 442 southern eclipsing binaries yielded 131stars with incorrect periods listed in the GCVS catalog
|
Program of Parallax Measurements from Space for the Nearest Eclipsing Binaries Not Available
|
The List of the Nearest and Bright Eclipsing Binaries from the HIPPARCOS Program Not Available
|
Statistics of categorized eclipsing binary systems Lightcurve shapes, periods, and spectral types The statistics of the light curve morphologies, eclipse depths, orbitalperiods, and spectral types of about 1000 eclipsing binary systems areexamined, after attempting to subdivide these binaries into variousbasic evolutionary categories. The applicability of statisticalcriteria, based on light curve morphologies and eclipse depths, for thecategorization of eclipsing binaries has been found more limited thanpreviously believed. In particular, EW-type light curves turn out to begood indicators of contact systems (though not conversely), while EA-and EB-type light curves have little physical significance. Moreover,the study reveals a strong deficit of short-period noncontact systems inthe whole spectral range, together with an underabundance of early-typecontact binaries (compared with the number of late-type contact pairs).Interestingly, the distribution of evolved Algol-type systems isshifted, on average, to periods longer than those of unevolved detachedsystems in the OB and early A spectral range (and to shorter periods inthe F spectral range).
|
A catalogue of parameters for eclipsing binaries Not Available
|
Photoelectrically-Neglected Eclipsing Binaries Not Available
|
Thirty Eclipsing Binaries Probably 100 ps Distant from the Sun Not Available
|
The velocity and space distribution of some types of variable stars (Errata: 17 310) Not Available
|
Die Bedeckungsveraenderlichen. Not Available
|
20 New Variable Stars in Harvard Map, No. 49. Not Available
|