Time-Dependent Variations of Accretion Disk
In dward nova we assume the primary star as a white dwarf and the secondary as the late type star which filled Roche lobe. Mass flow from the secondary star leads to the formation of thin accretion disk around the white dwarf. We use the α parameter as viscosity to maintain the disk form and propose...
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| Hlavní autoři: | , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
The Korean Space Science Society
1987-06-01
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| Edice: | Journal of Astronomy and Space Sciences |
| On-line přístup: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1987/v4n1/OJOOBS_1987_v4n1_11.pdf |
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