125 citations · 333 across the 12 of their papers we have counts for
14 papers · 1 filter
Forward Modeling of the Sct Star V1790 Ori: , , Resolution and Non-adiabatic Effects
Xiaoya Sun, Antonio García Hernández, Zhaoyu Zuo +5
We investigate the role of large separation, rotational correction order, structural resolution, and non-adiabatic effects in modelling the rotating Scuti star V1790 Ori. From…
Intermediate-mass stars and the origin of the gas-giant planet-metallicity correlation
J. Maldonado, G. M. Mirouh, I. Mendigutía +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…
The PL diagram for Sct stars: back in business as distance estimators
A. García Hernández, J. Pascual-Granado, M. Lares-Martiz +4
In this work, we focus on the period-luminosity relation (PLR) of Sct stars, in which mode excitation and selection mechanisms are still poorly constrained, and whose structure…
Dating young open clusters using delta Scuti stars. Results for Trumpler 10 and Praesepe
D. Pamos Ortega, G. M. Mirouh, A. García Hernández +2
Aims. The main goal of this work is to date young open clusters using Sct stars. Seismic indices such as the large separation and the frequency at maximum power can help to con…
Spectroscopic detection of Altair's non-radial pulsations
M. Rieutord, P. Petit, D. Reese +4
Context: Rapid rotation is a common feature of early-type stars but which remains a challenge for the models. The understanding of its effect on stellar evolution is however impera…
Forward modelling and the quest for mode identification in rapidly-rotating stars
Giovanni Marcello Mirouh
Asteroseismology has opened a window on the internal physics of thousands of stars, by relating oscillation spectra properties to the internal physics of stars. Mode identification…