Accretion Disks with a Cloudy Sky-photon Floater
Accretion Disks with a Cloudy Sky-photon Floater
复制标题
带有阴天光子浮子的吸积盘
DOI:
10.1093/pasj/48.1.89
复制
发表时间:
1996
影响因子:
2.3
通讯作者:
J. Fukue
中科院分区:
文献类型:
--
作者:
J. Fukue
Materials rotating above/below an accretion disk around a central object suffer from the influence of the strong radiation fields of the disk as well as the gravity of the central object. We find that there exists a critical floating height where the vertical gravity of the central object is balanced by the radiation force from the disk, and the materials are photon-floating there. The critical floating height is detemined by the disk effective luminosity reff, which is defined by reff = (CT/CTT)(mp/m)(Ld/LE), where CT and m are the material cross-section and mass, respectively, CTT and m p the Thomson cross-section and the proton mass, respectively, and Ld and LE the disk luminosity and the Eddington luminosity, respectively. For small r eff or large r (» z) the critical floating height ZF is expressed as ZF rv 3 rinreff, where rin is the inner radius of the disk. The astrophysically important point is that this critical floating height is dynamically stable; hence, materials, such as gas clouds or dust or artificials, suffering from the radiation field of the disk drift toward this floating height. Such floating clouds - photon floaters - above/below the disk partially occults the disk. If the disk sky is cloudy, the observed luminosity becomes irregular. Futhermore, if a cloudy sky is present, the emitted spectrum would be remarkably modified due to reprocessing. A cloudy sky would also produce absorption/emission features. In addition, since the radiation from the disk is scattered by floating clouds at a critical floating height, the disk appears as if its thickness had become ZF. The weather environment, such as a cloudy or dusty sky, changes the disk appearance significantly.