... Laboratory and theoretical modelling of the UV bump on the interstellar extinction ... number of different explanations of the UV bump (both successful and failed) using ...
... Using in the PNe's models the UV line intensities, planned to b e obtained with a help of WSO-UV observatory let us to determine the precision element abundances. ...
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Ссылки http://www.astro.spbu.ru/staff/afk/Papers/2008/MilanovaKholtygin_UVuniR.pdf -- 289.4 Кб -- 19.11.2010 Похожие документы
... Using in the PNe's models the UV line intensities, planned to be obtained with a help of WSO-UV observatory let us to determine the precision element abundances ...
... and spectropolarimetry in the optical and UV are extended to include regions su ... was restricted largely to optical and UV wavelengths as the high signal to noise ...
... R nQdr UV (11) where n is the density of scatterers, Q is the cross section of scatterers, and RUV is the UV photosphere ... L L M o = c c 4m R (25) UV from which we deduce that L 1 · o = 2R c 4 UV m (26) Explicitly comparing the momentum delivery ...
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Ссылки http://www.astro.spbu.ru/staff/afk/Papers/2004/MomProbl-04.pdf -- 111.3 Кб -- 19.11.2010 Похожие документы
... This is due to UV-radiation from hot, shor t-lived (< 108 yr) massive stars. ... The UV spectrum of sources at high z is also subject to additional opacity owing to ...