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Miloslav Dubec 《Astrophysics and Space Science》1991,175(2):207-213
A theory of gravitation in a flat space is briefly described, which gives a completely new view on cosmological problems. Instead of expansion of the Universe, a contraction of bodies and clusters is obtained. This theory excludes the closed solutions as non-physical ones and gives a simple condition for the stability of gravitationally-bounded systems with respect to cosmological gravitational field. 相似文献
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Zdeněk Mikulášek Marek Wolf Miloslav Zejda Petra Pecharová 《Astrophysics and Space Science》2006,304(1-4):363-365
We present two methods for the determination of moments of extrema and their errors appropriate for the analysis of light variations of variable objects. The method I is suitable for determination of times of extrema of non-periodical variables or objects, whose light curves vary. The method II is apt for O-C analyses of objects whose light curves are more or less repeating. Both methods are displayed on the analysis of BL Cam light variations and compared with the Kwee-van Woerden method. 相似文献