Tatsuya Yoshida

most citedLess effective hydrodynamic escape of H

_{2}

-H

_{2}

O atmospheres on terrestrial planets orbiting pre-main sequence M dwarfs

32 citations · 34 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.EP2023★ 2 cited

Strong depletion of $^{13}$ C in CO induced by photolysis of CO $_{2}$ in the Martian atmosphere calculated by a photochemical model

Tatsuya Yoshida, Shohei Aoki, Yuichiro Ueno +7

The isotopic signature of atmospheric carbon offers a unique tracer for the history of the Martian atmosphere and the origin of organic matter on Mars. Photolysis of CO $_{2}$ is kn…

astro-ph.EP2022★ 32 cited

Less effective hydrodynamic escape of H $_{2}$ -H $_{2}$ O atmospheres on terrestrial planets orbiting pre-main sequence M dwarfs

Tatsuya Yoshida, Naoki Terada, Masahiro Ikoma +1

Terrestrial planets currently in the habitable zones around M dwarfs likely experienced a long-term runaway greenhouse condition because of a slow decline in host-stellar luminosit…

Strong depletion of 13C in CO induced by photolysis of CO2​ in the Martian atmosphere calculated by a photochemical model

Less effective hydrodynamic escape of H2​-H2​O atmospheres on terrestrial planets orbiting pre-main sequence M dwarfs

Strong depletion of $^{13}$ C in CO induced by photolysis of CO $_{2}$ in the Martian atmosphere calculated by a photochemical model

Less effective hydrodynamic escape of H $_{2}$ -H $_{2}$ O atmospheres on terrestrial planets orbiting pre-main sequence M dwarfs