Doppler-free Saturated Absorption Spectroscopy By Priyanka Nandanwar.
E R(nr) non-resonant reflection
Stellar Winds and Mass Loss
Doppler-free Saturated Absorption Spectroscopy
E R(nr) non- resonant reflection (resonant) atomic response windo w dilute vapou r I R = | E R(nr) + E at | ² (non-resonnant) reflection at the interface.
Galactic Gas Kinematics and High Velocity Clouds at z~1
Stellar Winds and Mass Loss Brian Baptista. Summary Observations of mass loss Mass loss parameters for different types of stars Winds colliding with the.
