activity
20032024
most citedProbing the properties of convective cores through g modes: high-order g modes in SPB and gamma Doradus stars

254 citations · 1.4k across the 29 of their papers we have counts for

collaborators

28 papers

astro-ph.SR2024★ 5 cited

Mixed-mode coupling in the Red Clump I. Standard single star models

Walter E. van Rossem, Andrea Miglio, Josefina Montalbán

The investigation of global, resonant oscillation modes in red giant stars offers valuable insights into their internal structures. In this study, we investigate in detail the info…

astro-ph.SR2014★ 1 cited

Are the stars of a new class of variability detected in NGC~3766 fast rotating SPB stars?

S. J. A. J. Salmon, J. Montalbán, D. R. Reese +2

A recent photometric survey in the NGC~3766 cluster led to the detection of stars presenting an unexpected variability. They lie in a region of the Hertzsprung-Russell (HR) diagram…

astro-ph.SR2014★ 1 cited

Asteroseismology of Massive Stars : Some Words of Caution

A. Noels, M. Godart, S. Salmon +3

Although playing a key role in the understanding of the supernova phenomenon, the evolution of massive stars still suffers from uncertainties in their structure, even during their…

astro-ph.SR2014★ 70 cited

KIC 3858884: a hybrid δ Sct pulsator in a highly eccentric eclipsing binary

C. Maceroni, H. Lehmann, R. da Silva +10

The analysis of eclipsing binaries containing non-radial pulsators allows: i) to combine two different and independent sources of information on the internal structure and evolutio…

astro-ph.EP2013★ 128 cited

Kepler-91b: a planet at the end of its life. Planet and giant host star properties via light-curve variations

J. Lillo-Box, D. Barrado, A. Moya +8

The evolution of planetary systems is intimately linked to the evolution of their host star. Our understanding of the whole planetary evolution process is based on the large planet…

astro-ph.SR2013★ 43 cited

CoRoT 102918586: a Gamma Dor pulsator in a short period eccentric eclipsing binary

C. Maceroni, J. Montalbán, D. Gandolfi +2

Pulsating stars in eclipsing binary systems are powerful tools to test stellar models. Binarity enables to constrain the pulsating component physical parameters, whose knowledge dr…