... in PNe of the Magellanic Clouds and the Galactic halo has been established ... Large spread 1( 1.45) 1(>1.45) <1.3 Thick disk Halo Bulge M, M 0.641.09 0.570.64 z ... of a metal-rich gas in the halo and the thin and thick disks (Matteucci 2008 ...
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Ссылки http://www.astro.spbu.ru/staff/afk/Papers/2009/MilanovaKholtygin2009E.pdf -- 791.2 Кб -- 19.11.2010 Похожие документы
... a background radio source intersects a galaxy halo with overdensity 1000 relative to ... Because the Sun is about 26 ± 3 pc away from the Galactic plane as inferred from ... roughly 6 kpc from Sgr A towards the Sun. ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/publications/articles/mnras2015_452,4274.pdf -- 954.6 Кб -- 24.02.2016 Похожие документы
... with the Halogen Occultation Experiment (HALOE) (Russell et al., 1993) aboard ... path was taken perpendicular to the rising sun to ensure uniform illumination of the ... which is a geometric effect as the sun appears first over the horizon at these ...
Network Working Group N. Haller Request for Comments: 2289 Bellcore Obsoletes: 1938 C. Metz Category: Standards Track Kaman Sciences Corporation P. Nesser Nesser & Nesser Consulting M. Straw Bellcore February 1998 A One-Time Password System Status of...
... CME - coronal mass ejection: to - First C2 Appearance; v - Linear Speed [km/s]; T - type: Halo and partial Halo; pa - Position Angle measured from Solar North in degrees (counter-clockwise); CME on LASCO CME - list: http://cdaw.gsfc.nasa.gov/CME_list ...
... The in-falling O-helium flux from dark matter halo is where Vh is velocity of Solar System relative to DM halo (220 km/s), VE is velocity of orbital motion of Earth (29.5 km/s) and is the local density of O-helium dark matter. ...