Outflows from Young Stars: Theory and Observation

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Recent observations have revealed that young stellar objects are associated with jet-like structures and Herbig-Haro objects emitting at wavelengths ranging from optical lines to radio continua. These phenomena are similar in scales and morphologies and have mostly comparable energetics dynamics and kinematics. Probing such phenomena observed at various wavelengths with self-consistent physical and radiative processes arising with an inner disk-wind driven magnetocentrifugally from the circumstellar accretion disk is a challenge for confronting the theory and observation of outflows. How such early outflow phase may play a role in forming planetary materials may help solve puzzles posed by meteorites. We will discuss the relevant observations theoretical foundations for modeling approaches magnetic structures and dynamical effects and the connection to the early solar system.

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