Evolution of accretion disks with mass evaporation during the quiescence of WZ Sge-type dwarf novae and X-ray novae
文献类型：期刊论文
| 作者 | Mineshige, S1,2; Liu BF(刘碧芳)2,3 ; Meyer, F2; Meyer-Hofmeister, E2
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| 刊名 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
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| 出版日期 | 1998 |
| 卷号 | 50期号:5页码:L5-L9 |
| 关键词 | accretion disks black holes evaporation stars : dwarf novae X-rays : stars |
| ISSN号 | 0004-6264 |
| 产权排序 | 第三完成单位 |
| 通讯作者 | Mineshige, S |
| 英文摘要 | We propose a new scenario for disk evolution during the quiescence of WZ Sge-type dwarf novae and X-ray novae. A hole created by evaporation of the inner disk material steadily expands towards larger radii, eventually removing thermally unstable portions of the disk. The disk is, however, not in a steady state, since a certain amount of angular momentum is continuously brought in by an incoming stream, whereas angular-momentum losses due to the evaporation and to the tidal action by a companion star are likely to be small in the quiescence. Accordingly, the total angular momentum of the disk monotonically increases, whereas an increase in the disk mass is somewhat slower because of the mass evaporation. This results in an expansion of the disk and an accumulation of mass in the outermost part of the disk. The quiescence will be terminated if a thermal instability is ignited before the disk expands to the critical radius for the 3:1 resonance between Kepler and orbital angular frequencies. If not, superhumps are expected during quiescence. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | INSTABILITY MODEL ; OUTBURSTS ; TRANSIENTS ; STARS ; TIME |
| 收录类别 | SCI |
| 原文出处 | http://pasj.oxfordjournals.org/content/50/5/L5 |
| 语种 | 英语 |
| WOS记录号 | WOS:000076649400001 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/4924]  |
| 专题 | 云南天文台_高能天体物理研究组 |
| 作者单位 | 1.Department of Astronomy, Kyoto University, Sakyo-ku, Kyoto 606-8502; Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85740 Garching bei München, Germany 2.Max-Planck-Institut fur Astrophysik, Karl-Schwarzschild-Str. 1, D-85740 Garching, Germany 3.Yunnan Observatory, Academia Sinica, P.O. Box 110, Kunming 65011, China |
| 推荐引用方式 GB/T 7714 | Mineshige, S,Liu BF,Meyer, F,et al. Evolution of accretion disks with mass evaporation during the quiescence of WZ Sge-type dwarf novae and X-ray novae[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,1998,50(5):L5-L9. |
| APA | Mineshige, S,Liu BF,Meyer, F,&Meyer-Hofmeister, E.(1998).Evolution of accretion disks with mass evaporation during the quiescence of WZ Sge-type dwarf novae and X-ray novae.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,50(5),L5-L9. |
| MLA | Mineshige, S,et al."Evolution of accretion disks with mass evaporation during the quiescence of WZ Sge-type dwarf novae and X-ray novae".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 50.5(1998):L5-L9. |
入库方式： OAI收割
来源：云南天文台
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