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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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Official URL: http://www.springerlink.com/content/p20260tn4ux38744/fulltext.pdf
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 |
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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 |
Deposited On: | 24 Jul 2012 11:45 |
Last Modified: | 26 Jun 2018 07:16 |
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