activity
20192026
most citedSpectral Energy Distribution of the First Galaxies: Contribution from Pre-Main-Sequence Stars

2 citations · 3 across the 5 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

5 papers · 1 filter

astro-ph.EP2026

Thermochemical constraints on a primordial-origin of gas-rich debris disks

H. Mitani, W. Ooyama, R. Nakatani +2

Recent observations have revealed gas-rich debris disks around intermediate-mass stars at ages of tens of Myr. The origin of this gas remains unclear: it may be primordial, retaine…

astro-ph.EP2026

Analytical modeling of helium absorption signals of isothermal atmospheric escape

Hiroto Mitani, Rolf Kuiper

Atmospheric escape driven by extreme ultraviolet (EUV) radiation is a critical process shaping the evolution of close-in exoplanets. Recent observations have detected helium triple…

astro-ph.EP20251 cited

Physically motivated analytic model of energy efficiency for EUV-driven atmospheric escape of close-in exoplanets

Hiroto Mitani, Riouhei Nakatani, Rolf Kuiper

Extreme Ultraviolet (EUV) driven atmospheric escape is a key process in the atmospheric evolution of close-in exoplanets. In many evolutionary models, the energy-limited mass-loss…

astro-ph.EP2024

Secret of Longevity: Protoplanetary Disks as a Source of Gas in Debris Disks

Wataru Ooyama, Riouhei Nakatani, Takashi Hosokawa +2

While protoplanetary disks (PPDs) are generally thought to disperse within several million years, recent observations have revealed gas in their older counterparts, debris disks. T…

astro-ph.EP2020

Atmospheric Escape of Close-in Giants around Hot Stars: Far-Ultraviolet Radiation and Photoelectric Heating Effect

Hiroto Mitani, Riouhei Nakatani, Naoki Yoshida

Atmospheric escape is an important process that controls the long-term evolution of close-in planets. We perform radiation hydrodynamics simulations of photo-evaporation of exoplan…