Nearly-uniform internal rotation of solar-like main-sequence stars revealed by space-based asteroseismology and spectroscopic measurements

O. Benomar, M. Takata, H. Shibahashi +2

The rotation rates in the deep interior and at the surface of 22 main-sequence stars with masses between $1.0$ and $1.6{\mathrm{M}}_{\odot }$ are constrained by combining asteroseismol…