|COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring.|
Thick and thin disk kinematics with RAVE and the solar motion
If you have a question about this talk, please contact ma557.
I present a kinematic analysis of the Galactic thin and thick disks based on RAdial Velocity Experiment (RAVE). Thin and thick disk components are considered as two distinct galactic populations and disentangled from their mixture with analytical and statistical method. The prospects and limitations of this method are explored with the use of photometric distances and proper motions and compared with a phase-space synthetic Galactic model. I deduced the components of the solar motion relative to the local standard of rest in the radial and vertical direction, the velocity lag of the thick disk and the components of the velocity dispersion tensor for the thin and thick disk in the meridional plane.
This talk is part of the Institute of Astronomy Seminars series.
This talk is included in these lists:
Note that ex-directory lists are not shown.
Other listsCambridge University Global Health Society Fitzwilliam Lunctime talks Methodology in design research
Other talksHigh-dimensional variable selection Non-suicidal self-injury: an important transdiagnostic symptom cluster? The Human Plague Resilience of biodiversity and ecosystem services to environmental change Tbc Clinical Systems Medicine in Acute Myeloid Leukemia and Beyond