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21.
Miloslav Zejda Zdeněk Mikulášek Marek Wolf Ondřej Pejcha 《Astrophysics and Space Science》2006,304(1-4):161-163
We have re-analyzed old photometric UBV data obtained by Papoušek et al. at Skalnaté Pleso, Slovakia (1967–1980) and Brno, Czech Republic (1976–1979) observatories and analyzed new own CCD measurements (Brno, 2003–2005). In both set of photometric data the oscillations in the vicinity of the primary minimum were found. The detected periods are compatible with the previously published ones. 相似文献
22.
Vincenc Vyskočil Miloslav Burda Reviewer T. Kolbenheyer 《Studia Geophysica et Geodaetica》1976,20(3):213-218
Summary This paper deals with the methods of computing three-dimensional density models of the Earth's crust. Formulae for the numerical computation are given and the individual procedures are evaluated from a numerical point of view. 相似文献
23.
Summary It has been proved that the formulae for determining the horizontal co-ordinates of the centre of gravity, derived by Gamburtsev in 1938 and adopted in many textbooks of gravimetry and other works, are not accurate. A method of estimating the co-ordinates of the centre of gravity of a disturbing body has been elaborated under the assumption that just the values of the vertical gradient of the disturbing gravitational potential in the xOy-plane are known. 相似文献
24.
Summary The Gaussian beam method is applied to vertical seismic profiling in 2-D and 3-D models. A simple approach to the computation of Gaussian beam seismograms in the vicinity of structural interfaces is proposed. The effects of (a) the radiation pattern of a point source, (b) noncausal attenuation, (c) transverse inhomogeneities in synthetic seismograms are studied on numerical examples.
m¶rt; a n unm ¶rt; mua u nuuau ¶rt; u m ¶rt; ¶rt;. nmm n¶rt;¶rt; am a mmu mm a¶rt;a. a nua ummuu a uam m (a) uu m umua, () nu nu u () nn ¶rt;¶rt;m.相似文献
25.
Miloslav Burda Vincenc Vyskočil Reviewer L. Kubáčková 《Studia Geophysica et Geodaetica》1973,17(4):300-305
Summary A review of the terms of functional analysis, which can be exploited for statistical treatment of geophysical fields, is given. The procedure for determining the statistical characteristics of the fields, defined by a single realization, which does not require the limiting assumption of homogeneity to be introduced, is outlined. 相似文献
26.
This note removes a misunderstanding in the interpretation of solutions of the equations of motion in Friedmann's model. 相似文献
27.
BH Cen is a short-period early-type binary with a period of 0.792 din the extremely young star-forming cluster IC 2944. New multi-color CCD photometric light curves in U, B, V, R and I bands are presented and are analyzed by using the Wilson-Devinney code. It is detected that BH Cen is a high-mass-ratio overcontact binary with a fill-out factor of 46.4% and a mass ratio of 0.89. The derived orbital inclination i is 88.9 degrees, indicating that it is a totally eclipsing binary and the photometric parameters can be determined reliably. By adding new eclipse times, the orbital period changes in the binary are analyzed. It is confirmed that the period of BH Cen shows a long-term increase while it undergoes a cyclic oscillation with an amplitude of A_3 = 0.024 d and a period of P_3 = 50.3 yr. The high mass ratio, overcontact configuration and long-term continuous increase in the orbital period all suggest that BH Cen is in the evolutionary state after the shortest-period stage of Case A mass transfer.The continuous increase in period can be explained by mass transfer from the secondary component to the primary one at a rate of˙M_2 = 2.8×10~(-6) M_⊙per year. The cyclic change can be plausibly explained by the presence of a third body because both components in the BH Cen system are early-type stars. Its mass is determined to be no less than 2.2 M_⊙at an orbital separation of about 32.5 AU. Since no third light was found during the photometric solution, it is possible that the third body may be a candidate for a compact object. 相似文献
28.
Several new times of minimum light recorded with photoelectric or CCD means have been gathered for the eccentric eclipsing
binary V889 Aql (P = 11.1 days, e = 0.37). Its O–C diagram is presented, and improved elements of the apsidal motion and the light-time effect (LITE) are given. We found a
long apsidal motion period of about 24 400 ± 2400 years and a period of the third body of about 52 ± 2 years. 相似文献
29.
Ondřej Pejcha David Motl Miloslav Zejda Karel Koss Jitka KudrnÁčovÁ Petr HÁjek Ladislav Šmelcer Pavol A. Dubovský Eva ŠafÁřovÁ Marek Wolf 《Astrophysics and Space Science》2005,296(1-4):285-288
We present ephemerides and solutions of one Algol-type (KZ Dra) and two overcontact systems (LR Cam and IM Vul) based on V(RI)C CCD observations obtained in the project Prosper (network of amateur observers). 相似文献
30.
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