most citedEchography of young stars reveals their evolution

65 citations · 138 across the 5 of their papers we have counts for

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astro-ph.SR2016★ 25 cited

The effects of near-core convective shells on the gravity modes of the subdwarf B pulsator KIC 10553698A

Hamed Ghasemi, Ehsan Moravveji, Conny Aerts +2

KIC 10553698A is a hot pulsating subdwarf B (sdB) star observed by the Kepler satellite. It exhibits dipole (l = 1) and quadrupole (l = 2) gravity modes with a clear period spacing…

astro-ph.SR2014

Asteroseismic Diagnostics for Semi-Convection in B Stars in the Era of K2

Ehsan Moravveji

Semi-convection is a slow mixing process in chemically-inhomogeneous radiative interiors of stars. In massive OB stars, it is important during the main sequence. However, the effic…

astro-ph.SR2014★ 26 cited

Detection of solar-like oscillations in the bright red giant stars Psc and Tau from a 190-day high-precision spectroscopic multisite campaign

P. G. Beck, E. Kambe, M. Hillen +35

Red giants are evolved stars which exhibit solar-like oscillations. Although a multitude of stars have been observed with space telescopes, only a handful of red-giant stars were t…

astro-ph.SR2014★ 65 cited

Echography of young stars reveals their evolution

K. Zwintz, L. Fossati, T. Ryabchikova +17

We demonstrate that a seismic analysis of stars in their earliest evolutionary phases is a powerful method to identify young stars and distinguish their evolutionary states. The ea…

astro-ph.SR2014★ 22 cited

Modelling of Sigma Scorpii, a high-mass binary with a Beta Cep variable primary component

A. Tkachenko, C. Aerts, K. Pavlovski +6

High-mass binary stars are known to show an unexplained discrepancy between the dynamical masses of the individual components and those predicted by models. In this work, we study…