... corona is an important parameter for the models of gravitational radiation of the Galaxy: its variation would cause a significant change of gravitational radiation from the galactic polar regions, which are mostly populated by stars from the galactic ...
... Irradiation / Winds and Outflows / Coronae / Jets, Microquasars / Supercritical ... structure of the accreting two-temperature corona and the transition to an ADAF A. R ...
... The isolines of the critical frequency on the ( l , b ) sky map are presented in Figure 42 for the realistic galactic model described above and 10 percent of the mass of the corona consisting of stars, seen by the -detector. ...
... up propagated by Alfven waves to the disk corona, where they can power a jet or a ... The Dynamic Corona of Accretion Disks . ... The spectral properties of accretion disk coronae are reviewed. ...
... If the disk has a hot corona, the main process in this corona will be the scattering of hard photons on free electrons; further, these photons can penetrate into sub-photospheric layers of the disk, where they can be absorbed [23, 51]. ...
... Authors: Thomas Preibisch . Comments: 8 pages, Review talk at the Conference "Coronae of Stars and Accretion Disks", Bonn, Germany, December 2006. ...
... Stellar Coronae The spectra of stellar coronae obtained with Chandra contain a large number of interesting emission line ... notice that the coronae of both stars have a multi-temperature structure and that the temperature of the corona of Capella is ...
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