Gómez De Castro, Ana Inés2023-06-202023-06-2020040004-640X10.1023/B:ASTR.0000045063.90537.28https://hdl.handle.net/20.500.14352/50072Analytical 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.engjournal articlehttps//doi.org/10.1023/B:ASTR.0000045063.90537.28http://www.springerlink.com/content/p20260tn4ux38744/fulltext.pdfrestricted access52T-tauri starYoung starsBp tauriVariabilityUltravioletOutflowsAurigaeModelMagnetic fields-starsPlanetary systemsFormation-circumstellar matter-starsMass-lossProtoplanetary discsISMJets and outflowsAstronomía (Matemáticas)21 Astronomía y Astrofísica