We compute a new generation of standard solar models (SSMs) that includes recent
updates on some important nuclear reaction rates and a more consistent treatment of the …

We substantially update the capabilities of the open source software package Modules for
Experiments in Stellar Astrophysics (MESA), and its one-dimensional stellar evolution …

In the era of large stellar spectroscopic surveys, there is an emphasis on deriving not only
stellar abundances but also the ages for millions of stars. In the context of Galactic …

We present the first APOKASC catalog of spectroscopic and asteroseismic data for dwarfs
and subgiants. Asteroseismic data for our sample of 415 objects have been obtained by the …

In helioseismology, there is a well-known offset between observed and computed oscillation
frequencies. This offset is known to arise from improper modeling of the near-surface layers …

We present the first 4π–three-dimensional (3D) simulation of the last minutes of oxygen shell
burning in an 18 M⊙ supernova progenitor up to the onset of core collapse. A moving inner …

We analyze the simulation result shown in Hotta & Kusano (2021) in which the solar-like
differential rotation is reproduced. The Sun is rotating differentially with the fast equator and …

The medium-l program of the Michelson Doppler Imager instrument on board SOHO
provides continuous observations of oscillation modes of angular degree, l, from 0 to∼ 300 …

We report the results of a magnetohydrodynamic (MHD) simulation of a convective dynamo
in a model solar convective envelope driven by the solar radiative diffusive heat flux. The …

Solar-type stars exhibit a rich variety of magnetic activity. Seeking to explore the convective
origins of this activity, we have carried out a series of global three-dimensional …