Stellar Dynamical Evolution on the Main Sequence from Kepler Data - Savita Mathur

Explore stellar dynamical evolution on the main sequence using Kepler data in this 29-minute conference talk from the Transport in Stellar Interiors (TRANSTAR-C21) Conference. Delve into radiation age relationships, rotation, magnetic activity, and methods for measuring rotation periods. Examine results on state radiation periods, activity, Raspberry numbers, flares, and mid-frequency continuum. Investigate saturation dips, rotation gaps, and spectral types, with a focus on sunlike stars. Analyze standard deviations, SPH relationships, and active regions. Gain insights into the latest findings on stellar physics and transport processes in stellar interiors, combining observational data, theoretical calculations, and stellar models.

Intro
Radiation Age Relationships
Rotation
Magnetic Activity
Measuring Rotation Period
Results
State Radiation Period
Activity
Raspberry Number
Flares
Mid Frequency Continuum
Saturation
Dip
Rotation Gap
Spectral Types
Sunlike Stars
Standard Deviation
SPH Relationship
Active Regions
Conclusions
Questions