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Model physics in low-mass solar-type stars: atomic diffusion and metallicity mixture
Benard Nsamba, Tiago L. Campante, Mário J. P. F. G. Monteiro +4
Using asteroseismic data from the Kepler satellite, we explore the systematic uncertainties arising from changes in the input physics used when constructing evolution models of sol…
Mode Classification in Fast-Rotating Stars using a Convolutional Neural Network: Model-Based Regular Patterns in Scuti Stars
Giovanni M. Mirouh, George C. Angelou, Daniel R. Reese +1
Oscillation modes in fast-rotating stars can be split into several subclasses, each with their own properties. To date, seismology of these stars cannot rely on regular pattern ana…
Asteroseismic modelling of solar-type stars: internal systematics from input physics and surface correction methods
B. Nsamba, T. L. Campante, M. J. P. F. G. Monteiro +4
Asteroseismic forward modelling techniques are being used to determine fundamental properties (e.g. mass, radius, and age) of solar-type stars. The need to take into account all po…
Mode identification in rapidly rotating stars from BRITE data
Daniel R. Reese, Marc-Antoine Dupret, Michel Rieutord
Apart from recent progress in Gamma Dor stars, identifying modes in rapidly rotating stars is a formidable challenge due to the lack of simple, easily identifiable frequency patter…