... The stars with initial masses leave a WD in the end of evoluiton, with the WD masses and chemical composition depending on the binary system's parameters. Stars with collapses to form NS of 1.4 M; when a BH with a mass of is formed, where is either the mass of the pre-collapsing star (in the case of low stellar wind mass-loss scenario), or the initial mass of the star (in teh case of the high stellar wind mass-loss scenario). ... In that case supercritical regimes with mass outflow may happen. ...

arxiv:0901.3779 Кандидат в субпарсековые системы двух сверхмассивных черных дыр (A Candidate Sub-Parsec Supermassive Binary Black Hole System) . ... Authors: Mark. R. Krumholz et al. arxiv:0901.0304 Изотропный гамма фон: альбедо из-за космических лучей от "мусора" в Солнечной системе? Isotropic gamma-ray background: cosmic-ray induced albedo from debris in the Solar system?) ... обзор arxiv:0901.1149 Обилия элементов в солнечной системе (Abundances of the elements in the solar system) . ...

previous next contents elements attributes index . ... Lines and Paragraphs . ... Elements that present text (alignment elements, font elements, style sheets, etc.) are discussed elsewhere in the specification. ... Many of these are typographic elements used in some applications to produce particular visual spacing effects. ... For this reason, authors should use appropriate elements and styles to achieve visual formatting effects that involve white space, rather than space characters. ...