Asteroseismic measurement of surface-to-core rotation in a main-sequence star*
We have discovered rotationally split core g-mode triplets and surface p-mode triplets and quintuplets in a terminal age main-sequence A star, KIC 11145123, that shows both δ Sct p-mode pulsations and γ Dor g-mode pulsations. This gives the first robust determination of the rotation of the deep core...
Main Authors: | Kurtz Donald W., Saio Hideyuki, Takata Masao, Shibahashi Hiromoto, Murphy Simon J., Sekii Takashi |
---|---|
Format: | Article |
Language: | English |
Published: |
EDP Sciences
2015-01-01
|
Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/201510101007 |
Similar Items
-
Asteroseismic probing of the internal structure of main-sequence stars
by: Miglio, Andrea
Published: (2007) -
Nonadiabatic analysis of rosette modes of oscillations in rotating stars and their contribution to angular momentum transport
by: Takata Masao, et al.
Published: (2015-01-01) -
Asteroseismic inferences from red-giant stars
by: Themeẞl, Nathalie
Published: (2019) -
The Asteroseismic Poltential of TESS: Exoplanet-Host Stars
by: Campante, T. L., et al.
Published: (2017) -
Finding binaries from phase modulation of pulsating stars with Kepler
by: Shibahashi Hiromoto, et al.
Published: (2017-01-01)