... 314 ­ 321 Non­LTE Line Formation for Fe I and Fe I I in the Atmospheres of A­F Typ e Stars Mashonkina L. Institute of Astronomy, Moscow, Russia Abstract. ... Non­LTE leads to the Fe II lines strengthening, however, the effect is small, such that the abundance correction is at the level of -0.01 to -0.03 dex over the whole range of stellar parameters being considered. ... 2 What is Meant by the Non­LTE Approach? ... For the Fe I lines, we obtained the mean non­LTE abundance log FeI = 7.56 ± 0.09. ...

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... Parameters used in the modeling of the radial-velocity curves of the optical component in the Roche model P ,days e i, µ f T kx A u ef f 1.700167412 0.0 80 ; 88 1.0 1.0 Orbital period Eccentricity Orbital inclination Degree of Roche lobe filling by the optical component Asynchronicity factor for the rotation of the optical component Effective temperature of the non-perturbed optical component Gravitational-darkening coefficient Ratio of the ... observed profile (Fig. ...

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• ЗЕМНОЕ ЯДРО КАК ВОЗМОЖНЫЙ ИСТОЧНИК ГРАВИТАЦИОННЫХ АНОМАЛИЙ

Journal of the Amateur Astronomers Association of New York July 2010 Volume 58 Number 7, ISSN 0146-7662 EYEPIECE every week since, except for a break during the winter months of December through March, and the inevitable cancellations due to overcast skies. ... It's not the dark surroundings--other AAA observing sites are much darker. ... We're neither at the center nor the edge of anything, be it solar system, galaxy, local group, galactic cluster or universe. ... So, why does time go only one way? ...

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Introduction to PLASMA ASTROPHYSICS (Selected 10 lectures) Boris V. Somov Astronomical Institute and Faculty of Physics Moscow State University Pushino-na-Oke, 2008 Contents Ab out These Lectures 1 Particles and Fields: Exact Self-Consistent Description 1.1 Liouville's theorem . . . . . . . . . . . . . . . . . . . 1.1.1 Continuity in phase space . . . . . . . . . 1.1.2 The character of particle interactions 1.1.3 The Lorentz force, gravity . . . . . . . . . 1.1.4 Collisional friction . . . . . . . . . . . .

26. http://www.astro-soc.odessa.ua/Program-2008.pdf

27. http://vega.inp.nsk.su/~inest/OCAAS/ocaas.pdf