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发表于 2025-3-27 00:18:53
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Torrid
发表于 2025-3-27 04:03:11
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议程
发表于 2025-3-27 06:57:51
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idiopathic
发表于 2025-3-27 10:43:14
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Foam-Cells
发表于 2025-3-27 17:18:42
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
发表于 2025-3-27 21:51:36
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cogitate
发表于 2025-3-27 22:21:50
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
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发表于 2025-3-28 05:06:55
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debacle
发表于 2025-3-28 07:48:20
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
发表于 2025-3-28 13:10:00
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