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Apparent Photosphere of Massive Accretion-Disk Winds
[摘要] Weexaminedtheobservationalappearanceofhighlyopticallythickwindsfromsupercriticalaccretiondisks,whileespeciallyfocusingontheshapeofa“photosphere”ofthewind.Whenamassivewindblowsfromanaccretiondisk,theopticaldepthofthewindmayexceedunityintheplace,whichishigherthanthescaleheightofthedisk.Ifsuchawindisrealized,theobservedlightmayhaveoriginatedfromthephotosphereofthewind,ratherthanfromthedisksurface.Wecalculatedtheapparentsurfaceofthephotosphere,wheretheobservedopticaldepthisunity,andcompareditwiththegeometryoftheaccretiondisk.Wefoundthatthewindphotospherecanexpandoverthediskscale-heightforsuper-Eddingtonmass-lossrates,butthelocationandappearanceofthephotospherestronglydependontheinclinationangleaswellasthemass-lossrate.Thisfactmayaffectontheinterpretationoflightcurvesingalacticeclipsingbinariesandrecentlywell-observedultraluminousX-raysources.
[发布日期]  [发布机构] 
[效力级别]  [学科分类] 天文学(综合)
[关键词] "accretion;accretion disks";"black hole physics";"stars: winds;outflows";"X-rays: stars" [时效性] 
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