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20112026
most citedPlanet Engulfment by ~1.5-3 Solar-Mass Red Giants

137 citations · 752 across the 31 of their papers we have counts for

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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

X-ray emission of F-type stars and its analogy with G-type stars

Takuma Shimura, Ikuyuki Mitsuishi, Masanobu Kunitomo +3

We conducted a systematic spectral study for single F-type main-sequence (MS) stars without significant X-ray outbursts to investigate X-ray spectral properties such as temperature…

astro-ph.SR2025★ 3 cited

Solar models with protosolar accretion and turbulent mixing

Masanobu Kunitomo, Gaël Buldgen, Tristan Guillot

(abridged) Recent analyses have reported low lithium but high beryllium abundances on the solar surface; however, standard solar models (SSMs) predict Li abundances that are ~30…

astro-ph.SR2025

The Future of Solar modelling: requirements for a new generation of solar models

Gael Buldgen, Gloria. Canocchi, Arthur. Le Saux +22

Helioseismology and solar modelling have enjoyed a golden era thanks to decades-long surveys from ground-based networks such as for example GONG, BiSON, IRIS and the SOHO and SDO s…

astro-ph.SR2024

Spin-down of solar-mass protostars in magnetospheric accretion paradigm

Shinsuke Takasao, Masanobu Kunitomo, Takeru K. Suzuki +2

Stellar spin is one of the fundamental quantities that characterize a star itself and its planetary system. Nevertheless, stellar spin-down mechanisms in protostellar and pre-main-…

astro-ph.SR2022★ 25 cited

Evidence of a signature of planet formation processes from solar neutrino fluxes

Masanobu Kunitomo, Tristan Guillot, Gaël Buldgen

Solar evolutionary models are thus far unable to reproduce spectroscopic, helioseismic, and neutrino constraints consistently, resulting in the so-called solar modeling problem. In…

astro-ph.SR2022★ 36 cited

Diagnosing FUor-like Sources: The Parameter Space of Viscously Heated Disks in the Optical and Near-IR

Hanpu Liu, Gregory J. Herczeg, Doug Johnstone +8

FU Ori type objects (FUors) are decades-long outbursts of accretion onto young stars that are strong enough to viscously heat disks so that the disk outshines the central star. We…

astro-ph.SR2020★ 21 cited

Investigation of coronal properties of X-ray bright G-dwarf stars based on the solar surface magnetic field -- corona relation

Shinsuke Takasao, Ikuyuki Mitsuishi, Takuma Shimura +4

We investigated the coronal properties of G-dwarf stars including the Sun over a wide range of X-ray luminosity ( to …

astro-ph.SR2020★ 5 cited

Four New Self-lensing Binaries from Kepler: Radial Velocity Characterization and Astrophysical Implications

Kento Masuda, Hajime Kawahara, David W. Latham +5

In Kawahara et al. (2018) and Masuda et al. (2019), we reported the discovery of four self-lensing binaries consisting of F/G-type stars and (most likely) white dwarfs whose masses…

astro-ph.SR2019★ 61 cited

Self-lensing Discovery of a White Dwarf in an Unusually Wide Orbit Around a Sun-like Star

Kento Masuda, Hajime Kawahara, David W. Latham +4

We report the discovery of the fifth self-lensing binary in which a low-mass white dwarf (WD) gravitationally magnifies its 15th magnitude G-star companion, KIC 8145411, during ecl…

astro-ph.SR2018★ 40 cited

Revisiting the pre-main-sequence evolution of stars II. Consequences of planet formation on stellar surface composition

Masanobu Kunitomo, Tristan Guillot, Shigeru Ida +1

We want to investigate how planet formation is imprinted on stellar surface composition using up-to-date stellar evolution models. We simulate the evolution of pre-main-sequence st…

astro-ph.SR2017★ 62 cited

Revisiting the pre-main-sequence evolution of stars I. Importance of accretion efficiency and deuterium abundance

Masanobu Kunitomo, Tristan Guillot, Taku Takeuchi +1

Recent theoretical work has shown that the pre-main-sequence (PMS) evolution of stars is much more complex than previously envisioned. Instead of the traditional steady, one-dimens…

astro-ph.SR2016★ 62 cited

From Birth to Death of Protoplanetary Disks: Modeling Their Formation, Evolution, and Dispersal

Shigeo S. Kimura, Masanobu Kunitomo, Sanemichi Z. Takahashi

Formation, evolution, and dispersal processes of protoplanetary disks are investigated and the disk lifetime is estimated. Gravitational collapse of a pre-stellar core forms both a…