... that is caused by an accretion disk with a large inner disk radius : The second is a ... disk spectrum shown in Figure 3 is speciпed by two parameters : (1) the temperature ...
... a complex spectral shape; a multicolor disk model, suitable for brighter ULXs, is ... 0.3 and 10.0 keV with an absorbed power-law model and an absorbed disk blackbody ...
... brown dwarfs that might be part of the thin disk stellar population, or the slightly puffier thick disk, or even the halo ... The coolest and faintest ones ought to be detectable in at least the thin disk if not the thick disk also. ...
... quasar accretion disks are reasonably well aligned with their galactic host disks,11 ... initial equilibrium disk models are constructed to be representative of disks at the ...
... luminosity, inconsistent with efficient disk accretion, there are other properties by which the Sombrero's nucleus differs from Seyfert 1 nuclei: (1) the latter exhibit Fe K emission lines produced in the accretion disk whose strength clearly increases ...
... by large column densities of gas and dust, obscuring the GRB afterglows (Groot et al ... forming regions where large quantities of gas and dust are present (e.g. Paczy'nski ...
... is derived from the Galactic stel lar model, which consists of the central spherical cluster, the central disk, the triaxial ellipsoidal GB and the Galactic disk (Muno et al. 2006, hereafter M06; Launhardt et al. 2002, here after L02; Kent et al. 1991 ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/papers/0805-draft-jaesub-xray_dist.ps -- 2015.5 Кб -- 12.06.2008 Похожие документы