... arXiv.org . ... Although great progress has been made in modelling the disk with radiative transfer models able to reproduce the spectral energy distribution (SED) of Herbig Ae stars, the constraints brought by images have not been yet fully exploited. Here, we are interested in checking if these new observational imaging constraints can be accounted for by predictions based on existing models of passive centrally irradiated hydrostatic disks made to fit the SEDs of the Herbig Ae stars. ...
... Key words: X-rays: stars; stars: neutron; magnetic fields; line: formation. в 1 1+z (n = 0, 1, 2, . ... Line profiles are shown for a continuum spectrum of the form of a power law with a high-energy exponential cutoff f (E ) = const. в E - в exp (-E / ) (XSPECs cutoffpl) and for different cutoff energies. fit (Fig. 4, bottom) was obtained for cylinder geometry, revealing a magnetic field strength of B = 2.95 в 1012 G, a viewing angle of µ = 0.76 and the plasma electron temperature of k Te = 3.4 keV....
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G41_Schoenherr01-07Feb07_16:54:04.pdf -- 385.0 Кб -- 07.02.2007 Похожие документы
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