| タイトル | The evolution of protoplanetary disks |
| 著者（英） | Ruden, Steven P. |
| 著者所属（英） | NASA Headquarters |
| 発行日 | 1993-01-01
1993 |
| 言語 | eng |
| 内容記述 | Accretion disks evolve by transferring angular momentum outwards, which allows mass to flow inwards onto the central object. The radial structure and time-dependent behavior of low-mass, Keplerian, viscous disks is analyzed. Potential mechanisms for the angular momentum transport in disks are reviewed. An evolutionary model of a low mass disk around a pulsar is presented. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 93A36441 |
| 権利 | Copyright |
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