activity
19982026
most citedAsteroseismic measurement of surface-to-core rotation in a main sequence A star, KIC 11145123

238 citations · 984 across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.SR2026

Solar Neutrino Flux Fluctuations Caused by Solar Gravity Modes

Yoshiki Hatta, Yuuki Nakano, Sho Sugama +3

We have evaluated fluctuations in neutrino fluxes caused by solar gravity (g) modes based on the analysis of linear adiabatic oscillation of a spherically symmetric star. We find t…

astro-ph.SR2025

High-order Gravity-mode Period Spacing Patterns of Intermediate-mass () Main-sequence Stars I. Perturbative Analysis

Yoshiki Hatta, Takashi Sekii

Theoretical study of high-order gravity-mode period spacing () pattern is relevant for the better understanding of internal properties of intermediate-mass ($1.5 \, M_\odot <…

astro-ph.SR2024

Inversion for Inferring Solar Meridional Circulation: The Case with Constraints on Angular Momentum Transport inside the Sun

Yoshiki Hatta, Hideyuki Hotta, Takashi Sekii

We have carried out inversions of travel times as measured by Gizon et al. (2020) to infer the internal profile of the solar meridional circulation (MC). A linear inverse problem h…

astro-ph.SR2023★ 5 cited

Detecting active latitudes of Sun-like stars using asteroseismic a-coefficients

Othman Benomar, Masao Takata, Michael Bazot +3

We introduce a framework to measure the asphericity of Sun-like stars using , and coefficients, and constrain their latitudes of magnetic activity. Systematic erro…

astro-ph.SR2021★ 6 cited

Bayesian rotation inversion of KIC 11145123

Yoshiki Hatta, Takashi Sekii, Othman Benomar +1

A scheme of Bayesian rotation inversion, which allows us to compute the probability of a model of a stellar rotational profile, is developed. The validation of the scheme with simp…

astro-ph.SR2021★ 17 cited

The two-dimensional internal rotation of KIC11145123

Yoshiki Hatta, Takashi Sekii, Masao Takata +1

The two-dimensional internal rotation of KIC11145123 has been inferred via asteroseismology. Based on the Optimally Localized Averaging method and a simple three-zone modeling of t…