G. Mirouh

collaborators

3 papers

astro-ph.SR2026

Forward Modeling of the $I^´$ Sct Star V1790 Ori: $I^ I^½$ , $I^c ◯$ , Resolution and Non-adiabatic Effects

Xiaoya Sun, Antonio GarcÃa HernÃ¡ndez, Zhaoyu Zuo +5

We investigate the role of large separation, rotational correction order, structural resolution, and non-adiabatic effects in modelling the rotating $I^´$ Scuti star V1790 Ori. From…

astro-ph.SR2026

Lithium and the evolution of intermediate-mass T Tauri and Herbig stars. Rotation, accretion, and planets

I. MendigutÃa, J. Campbell-White, B. Montesinos +9

(Abridged) We contribute to our understanding of the evolution of young intermediate-mass stars by providing a comprehensive analysis of their lithium (Li) content. A sample of 71…

astro-ph.SR2025

Intermediate-mass stars and the origin of the gas-giant planet-metallicity correlation

J. Maldonado, G. M. Mirouh, I. MendigutÃa +3

The number of known planets around intermediate-mass stars (1.5 M $_{⊙}$ < M $_{⋆}$ < 3.5 M $_{⊙}$ ) is rather low. We aim to test whether the correlation between the metal…

Forward Modeling of the I^´ Sct Star V1790 Ori: I^I^½, I^c◯, Resolution and Non-adiabatic Effects

Lithium and the evolution of intermediate-mass T Tauri and Herbig stars. Rotation, accretion, and planets

Intermediate-mass stars and the origin of the gas-giant planet-metallicity correlation

Forward Modeling of the $I^´$ Sct Star V1790 Ori: $I^ I^½$ , $I^c ◯$ , Resolution and Non-adiabatic Effects