Re-condensation from an ADAF into an inner disk: the intermediate state of black hole accretion? | |
Meyer, F1; Liu BF(刘碧芳)2; Meyer-Hofmeister, E1; Meyer, F (reprint author), Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85740 Garching, Germany. | |
发表期刊 | ASTRONOMY & ASTROPHYSICS |
2007-02 | |
卷号 | 463期号:1页码:1-9 |
DOI | 10.1051/0004-6361:20066203 |
产权排序 | 第2完成单位 |
收录类别 | SCI ; EI |
关键词 | Black Hole Physics Accretion X-rays : Binaries Accretion Disks Stars : Individual : Cyg X-1 |
摘要 | Context. Accretion onto galactic and supermassive black holes occurs in different modes, which are documented in hard and soft spectral states, commonly attributed to an advection-dominated flow (ADAF) inside a truncated disk and standard disk accretion, respectively. At the times of spectral transition an intermediate state is observed, for which the accretion flow pattern is still unclear. Aims. We analyze the geometry of the accretion flow when the mass flow rate in the disk decreases (soft/hard transition) and evaporation of gas into the coronal flow leads to disk truncation. Methods. We evaluate the physics of an advection-dominated flow affected by thermal conduction to a cool accretion disk underneath. Results. We find re-condensation of gas from the ADAF into the underlying inner disk at distances from the black hole and at rates, that depend on the properties of the hot ADAF and vary with the mass accretion rate. This sustains an inner disk for longer than a viscous decay time after the spectral transition occurred, in accordance with the spectra that indicate cool gas in the neighborhood of the accreting black hole. The model allows us to understand why Cyg X-1 does not show hysteresis in the spectral state transition luminosity that is commonly observed for X-ray transient sources. Conclusions. Our results shed new light on the complex mass flow pattern during spectral state transition. |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 0004-6361 |
URL | 查看原文 |
WOS记录号 | WOS:000243941900001 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | X-RAY BINARIES ; ADVECTION-DOMINATED ACCRETION ; ACTIVE GALACTIC NUCLEI ; ALL-SKY MONITOR ; SPECTRAL STATE ; TEMPORAL PROPERTIES ; XTE J1650-500 ; CORONAL FLOW ; LIGHT CURVES ; DWARF NOVAE |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/4956 |
专题 | 高能天体物理研究组 |
通讯作者 | Meyer, F (reprint author), Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85740 Garching, Germany. |
作者单位 | 1.Max-Planck-Institut für Astrophysik, Karl- Schwarzschildstr. 1, 85740 Garching, Germany 2.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, PO Box 110, Kunming 650011, PR China |
推荐引用方式 GB/T 7714 | Meyer, F,Liu BF,Meyer-Hofmeister, E,et al. Re-condensation from an ADAF into an inner disk: the intermediate state of black hole accretion?[J]. ASTRONOMY & ASTROPHYSICS,2007,463(1):1-9. |
APA | Meyer, F,Liu BF,Meyer-Hofmeister, E,&Meyer, F .(2007).Re-condensation from an ADAF into an inner disk: the intermediate state of black hole accretion?.ASTRONOMY & ASTROPHYSICS,463(1),1-9. |
MLA | Meyer, F,et al."Re-condensation from an ADAF into an inner disk: the intermediate state of black hole accretion?".ASTRONOMY & ASTROPHYSICS 463.1(2007):1-9. |
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