Gómez de Castro, Ana Inés (2004) Magnetic activity and the interaction between the stellar magnetosphere and the accretion disk. Astrophysics and space science, 292 . pp. 561-572. ISSN 0004-640X
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Abstract
Analytical and numerical analysis of the interaction between the magnetosphere of the Pre-Main-Sequence (PMS) stars and accretion disks are converging to a robust, fundamental mechanism for jet formation. They provide a reasonably solid base-line to explain the current observations on the formation of solar-like stars. In this summary, the connection between observations and this paradigm are reviewed critically and some observational tests proposed.
| Item Type: | Article |
|---|---|
| Uncontrolled Keywords: | T-tauri star; young stars; bp tauri; variability; ultraviolet; outflows; aurigae; model; magnetic fields-stars : formation-circumstellar matter-stars : mass-loss; planetary systems : protoplanetary discs; ISM : jets and outflows |
| Subjects: | Sciences > Mathematics > Astronomy |
| ID Code: | 16063 |
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| Deposited On: | 24 Jul 2012 13:45 |
| Last Modified: | 24 Jul 2012 13:45 |
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