Titlebook: Light Curve Modeling of Eclipsing Binary Stars; E. F. Milone Conference proceedings 1993 Springer-Verlag New York, Inc. 1993 Periastron.Va

全部逛商店

Torrid

議程

idiopathic

Foam-Cells

Some Comments on Light Curve Solution of Eclipsing Binaries,s lead to large deviations in the solution. A stable solution of the problem needs knowledge of so-called “a priori” physical information about the solution. The algorithms of the solving of ill-posed problems based on application of “a priori” information (so-called regularisation algorithms) have

BOON

cogitate

Binary Star Rotation from Line Profiles,erential correction method while F.(simplex) refers to the value obtained from the simplex method. F.(lc) is the photometric F1 value. The published spectroscopic F. values in Table 1 are averages found by Van Hamme and Wilson (1990, Ai 100, 1981) from the listed references. The last column in Table

來自于

debacle

Light Synthesis Modeling of Close Binary Stars,ntation of the observations than the hot secondary model..Sparse observational data at 330, 250, and 220 nm from the Astronomical Netherlands Satellite have historically been interpreted to provide support for the starspot model. However, simulation of the individual light curves demonstrates inabil

Foment