Optical Light Curves of Luminous Eclipsing Black Hole X-Ray Binaries

Watarai Ken-ya; Fukue Jun

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Optical Light Curves of Luminous Eclipsing Black Hole X-Ray Binaries

机译：夜视黑洞X射线二元图像的光曲线

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Weexaminedoptical$$V$$-bandlightcurvesinluminouseclipsingblackholeX-raybinaries,usingasupercriticalaccretion/outflowmodelthatismorerealisticthantheformerlyusedones.Inordertocomputethetheoreticallightcurveinthebinarysystem,wedidnotonlyapplytheglobalanalyticsolutionofthedisk,butalsoincludedtheeffectofopticallythickoutflow.Wefoundthatthedepthofeclipseofthecompanionstarbythediskchangeddramaticallywhenincludingtheeffectoftheoutflow.Duetotheeffectofoutflow,wecouldreproducetheopticallightcurvefortypicalbinaryparametersinSS433.Ourmodelwithanoutflowvelocityof$$vsim$$3000kms$$^{-1}$$couldfitthewholeshapeoftheaveraged$$V$$-bandlightcurveinSS433,butwefoundapossibleparameterrangeconsistentwithobservations,suchas$$dot{M}sim$$5000a€“10000$$L_{ mE}/c^2$$(with$$L_{ mE}$$beingtheEddingtonluminosityand$$c$$beingthespeedoflight)and$$T_{ mC}=$$10000$$gt$$Ka€“14000Kfortheaccretionrateanddonorstartemperature,respectively.Furthermore,webrieflydiscussobservationalimplicationsforultraluminousX-raysources.

机译：Weexaminedoptical $$ V $$ - bandlightcurvesinluminouseclipsingblackholeX-raybinaries，usingasupercriticalaccretion / outflowmodelthatismorerealisticthantheformerlyusedones.Inordertocomputethetheoreticallightcurveinthebinarysystem，wedidnotonlyapplytheglobalanalyticsolutionofthedisk，butalsoincludedtheeffectofopticallythickoutflow.Wefoundthatthedepthofeclipseofthecompanionstarbythediskchangeddramaticallywhenincludingtheeffectoftheoutflow.Duetotheeffectofoutflow，wecouldreproducetheopticallightcurvefortypicalbinaryparametersinSS433.Ourmodelwithanoutflowvelocityof $$ VSIM $$ 3000kms $$ ^ { - 1} $$ couldfitthewholeshapeoftheaveraged $$ V $$ - BandlightcurveinSS433，但是我们发现一个可行的参数范围与观察值一致，例如$$ dot {M} sim $$ 5000a€“ 10000 $$ L_ {mE} / c ^ 2 $$（with $$ L_ {mE} $$ beingtheEddingtonluminosity and $$ c $ beingthelightlightlight）和$ $ T_ {mC} = $$ 10000 $$ gt $$ Ka€“分别为14000K的吸积率和供体星温度。此外，webriefly讨论了观察性暗示性X射线源。

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《PASJ: Publications of the Astronomical Society of Japan》 |2010年第2期|共页
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Watarai Ken-ya; Fukue Jun;
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1. Optical Light Curves of Luminous Eclipsing Black Hole X-Ray Binaries [J] . Ken-ya WATARAI, Jun FUKUE PASJ: Publications of the Astronomical Society of Japan . 2010,第2期

机译：夜视黑洞X射线二元图像的光曲线
2. THE 2002 OUTBURST OF THE BLACK HOLE X-RAY BINARY 4U 1543-47: OPTICAL AND INFRARED LIGHT CURVES [J] . M. M. BUXTON, C. D. BAILYN The Astrophysical journal . 2004,第2PT1期

机译：黑洞X射线二进制4U 1543-47的2002年爆发：光学和红外光曲线
3. The 2002 Outburst of the Black Hole X-Ray Binary 4U 1543–47: Optical and Infrared Light Curves [J] . M. M. Buxton, C. D. Bailyn The Astrophysical journal . 2004,第2期

机译：2002年黑洞X射线二进制4U 1543-47的爆发：光学和红外光曲线
4. The Eclipsing Black Hole X-ray Binary M33 X-7: Understanding the Current Properties [C] . Francesca Valsecchi, Bart Willems, Tassos Fragos, Workshop on Hot and Cool: Bridging Gaps in Massive-Star Evolution . 2010

机译：Ecliping Black Hole X射线二进制M33 X-7：了解当前的属性
5. Detailed atmosphere calculations of accretion disks around intermediate mass black holes, and their application to observations of ultra-luminous X-ray sources [D] . Hui, Yawei 2009

机译：中间质量黑洞周围吸积盘的详细大气计算，及其在超发光X射线源观测中的应用
6. Disks around merging binary black holes: From GW150914 to supermassive black holes [O] . Abid Khan, Vasileios Paschalidis, Milton Ruiz, -1

机译：合并二进制黑洞周围的磁盘：从GW150914到超大质量黑洞
7. Optical Light Curves of Luminous Eclipsing Black Hole X-ray Binaries [O] . Watarai, Ken-ya, Fukue, Jun 2010

机译：发光遮蔽黑洞X射线二元光学光学曲线

Optical Light Curves of Luminous Eclipsing Black Hole X-Ray Binaries

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