RT Journal Article
T1 Magnetic activity and the interaction between the stellar magnetosphere and the accretion disk
A1 Gómez De Castro, Ana Inés
AB 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.
PB Springer
SN 0004-640X
YR 2004
FD 2004
LK https://hdl.handle.net/20.500.14352/50072
UL https://hdl.handle.net/20.500.14352/50072
LA eng
DS Docta Complutense
RD 5 abr 2025