... collision abundances of carbon ions in the framework of the accepted line intensity fitting method has shown that the fitted abundances are optimal in the sense that the differences between the observed and the calculated intensities both for ...
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Ссылки http://www.astro.spbu.ru/staff/afk/Papers/1998/InhomPNe1998.pdf -- 434.1 Кб -- 19.11.2010 Похожие документы
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Ссылки http://www.astro.spbu.ru/staff/afk/Papers/2009/MilanovaKholtygin2009E.pdf -- 791.2 Кб -- 19.11.2010 Похожие документы
... 12) Here the dimensional constant A0 = 8.6287 10 by ij = -6 cm3 s-1 K1/2 and ij is the collision strength averaged over a maxwellian electron velocity distribution, usually referred to as the effective collision strength. ...
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Ссылки http://www.astro.spbu.ru/staff/afk/Papers/2008/Kholtygin2008NeTediagnE.pdf -- 157.1 Кб -- 19.11.2010 Похожие документы
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Ссылки http://www.astro.spbu.ru/Sobolev100/sites/default/files/Sobolev-100.pdf -- 2775.2 Кб -- 02.10.2015 Похожие документы
... around stellar objects and active galactic nuclei I. Computational methods and ... around evolved stars, starburst galaxies, or tori around active galactic nuclei ... regions, envelopes, and evolved stars, or tori around active galactic nuclei ...
... into account when modeling Galactic-dust emission properties, which are calculated ... Collisions of dust grains with atoms and molecules cause rapid grain rotation with ...
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Ссылки http://www.astro.spbu.ru/staff/ilin2/INTAS/P3-SPB1/PUBL/TEXT/vs-pazh.pdf -- 473.3 Кб -- 19.11.2010 Похожие документы