... conductivity tensor was evaluated under the assumption that dust grains have settled towards the midplane of the disc, an ... In a final part of this project I computed these solutions for a disc where dust grains are well mixed with the gas phase. ...
... Even the circumstances of the observation were similar to de Cheseaux's, but in the case of P1, we know these are not separate tails but structures within a single dust tail (be these structures synchrones or striae). ...
... 48: The Effect of Dust Geometry on the LyЮБ Output of Galaxies . ... of the Parkes sample of flat-spectrum radio sources: dust in radio-loud quasars ... ASA, 13, 207-211 . 15: Dust-reddened Quasars . ...
... type dust (rejected at the 3.4 p conпdence level) and grayer dust (grain size [ 0.1 ... dust rather than a cosmological constant were the sole reason that z B 0.5 SNe Ia ...
... Consider a dust cloud of thickness d, composed of dust grains, each of radius r. There are n dust grains per unit volume, throughout the cloud. ...
... just like local starburst galaxies, and dust is remarkably good at blocking optical ... This technique only finds young, dustfree galaxies, but what other sorts of ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight.ps -- 153.9 Кб -- 30.08.1998 Похожие документы
... Consider a dust cloud of thickness d, composed of dust grains, each of radius r. There are n dust grains per unit volume, throughout the cloud. ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L06/Approximations.pdf -- 219.3 Кб -- 04.03.2011 Похожие документы