On the Dynamical Structure of the Jet System in the Disk with the Keplerian Rotation
The classical sloar wind theory proposed by Parker(1963) explains well the dynamics of the wind pheonomena such as stellar wind accretion disk. While the stellar wind system like the solar wind has the spherically symmetric wind structure, there are various jet phenomena which collimate the system i...
| Main Authors: | , , , |
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| Format: | Article |
| Language: | English |
| Published: |
The Korean Space Science Society
1989-06-01
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| Series: | Journal of Astronomy and Space Sciences |
| Online Access: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1989/v6n1/OJOOBS_1989_v6n1_17.pdf |