... The total gas mass in the plume (7x10 8 M sun ) and tail (1x10 9 M sun ) is about three times that in the core of M86, which supports the scenario where most of the gas was stripped rapidly and recently. ...
... 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 . ...
... 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. ...
... Nuture of Quiet Sun Radiation. Distribution of Radio-Brightness on the Disk. ... Refraction of the R-Waves in the Solar Atmosphere. UV- and X-Radiation of the Sun. ... Gas Halo of the Galaxy. The Source of the Interstellar Medium Ionization. ...
... and near Earth space after powerful explosive releases of energy on the Sun ... are accelerated and propagate on the Sun and in the interplanetary medium and in ... SPEs and the accompanying phenomena on the Sun during cycles 2124, paying attention ...
... Andriyenko O.V. Osipov S.N. On variations of features of 525.02 and 525.06 nm lines in the sun-as- a-star spectrum. Abstr. ... p.333 . 3070 . Silich S.A. Tonorio-Tagle G. Gas outflows in Starburst dwarf galaxies with extended halos. Abstr. ...
... the Galactic halo following that of the dark mat- ter (which is the case for the superheavy darkmatter (SHDM) particles and some of topological defects) predict [4] the Galactic center-anticenter asymmetry due to the non-central position of the Sun in the ...
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Ссылки http://cosrad.sinp.msu.ru/experiments/tus/doc/global2007.pdf -- 136.8 Кб -- 19.03.2008 Похожие документы
... increase in solar activity in both the northern and southern hemispheres of the sun ... high-velocity stars in the Galactic halo; dwarf carbon stars, including the search ...
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Ссылки http://www.princetonastronomy.org/newsletters/03_2010sidereal.pdf -- 971.3 Кб -- 04.03.2010 Похожие документы