... The Galactic potential is assumed to be axisymmetric consisting of disk, buldge and halo parts (see Paczynski 1990). ... The Sun was assumed to be at the Galactic plane at a distance 8.5 kpc from the center of the Galaxy. 2.2. ...
... is assumed to be axisymmetric, resulting from the sum of three contributions: the disk, bulge and halo (see Paczynski 1990 ... The Sun is in the Galactic plane at a distance 8.5 kpc from the Galactic Center. 2.3. ...
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Ссылки http://xray.sai.msu.ru/~polar/html/publications/belt_aa/final.ps -- 304.3 Кб -- 02.04.2003 Похожие документы
... It involves six components: nucleus, bulge, halo, disk, flat component and corona (see Table 12 ). ... the density of population II stars in the vicinity of the Sun, the galactic rotation curve and the dynamics and distribution of ...
... S only for stars in some vicinity of the Sun (two values were used: 500 pc and 5 kpc ... inside 5 kpc sphere around the Sun and distributions of temperature, velocity and ...
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Ссылки http://xray.sai.msu.ru/~polar/html/publications/LogNLogS_AATr/new_big1.ps -- 174.4 Кб -- 04.01.2002 Похожие документы
... Discovery of a Metal-poor L Dwarf with Halo Kinematics) . Authors: Adam J. Burgasser et al. Экзопланеты . ... What Fraction of Sun-like Stars have Planets?) . Authors: Charles H. Lineweaver, Daniel Grether . ...
... astro-ph/0605026 Форма гало Млечного Пути (The Shape of the Milky Way Halo) . Authors: M. Fellhauer et al. ... будет и про белые карлики). astro-ph/0605414 Транзитная планета у солнцеподобной звезды (A Transiting Planet of a Sun-like Star ...