Forward modelling and the quest for mode identification in rapidly rotating stars
Asteroseismology has opened a window on the internal physics of thousands of stars, by relating oscillation spectra properties to the internal physics of stars. Mode identification, namely the process of associating a measured oscillation frequency to the corresponding mode geometry and properties,...
Main Author: | Giovanni M. Mirouh |
---|---|
Format: | Article |
Language: | English |
Published: |
Frontiers Media S.A.
2022-10-01
|
Series: | Frontiers in Astronomy and Space Sciences |
Subjects: | |
Online Access: | https://www.frontiersin.org/articles/10.3389/fspas.2022.952296/full |
Similar Items
-
2D modelling of pulsating stars with rapid rotation
by: Daniel Roy Reese
Published: (2022-09-01) -
Kepler main-sequence solar-like stars: surface rotation and magnetic-activity evolution
by: Ângela R. G. Santos, et al.
Published: (2024-03-01) -
Cracking Strange Stars by Torsional Oscillations
by: Francesco Tonelli, et al.
Published: (2018-02-01) -
Dynamics of star clusters/
by: International Astronomical Union Symposium (113th : 1984 : Princeton, New Jersey), et al.
Published: (1985) -
Asteroseismic Signature of a Large Active Region
by: Emanuele Papini, et al.
Published: (2019-12-01)