activity
20102016
most citedPhysics Of Eclipsing Binaries. II. Towards the Increased Model Fidelity

326 citations · 729 across the 9 of their papers we have counts for

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Showing 2014Show all

5 papers · 1 filter

astro-ph.SR201426 cited

The blue-edge problem of the V1093 Her instability strip revisited using evolutionary models with atomic diffusion

S. Bloemen, Haili Hu, C. Aerts +5

We have computed a new grid of evolutionary subdwarf B star (sdB) models from the start of central He burning, taking into account atomic diffusion due to radiative levitation, gra…

astro-ph.SR201463 cited

On the use of the Fourier Transform to determine the projected rotational velocity of line-profile variable B stars

C. Aerts, S. Simon-Diaz, P. J. Groot +1

The Fourier Transform method is a popular tool to derive the rotational velocities of stars from their spectral line profiles. However, its domain of validity does not include line…

astro-ph.SR201426 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.SR201420 cited

Discovery of binarity, spectroscopic frequency analysis, and mode identification of the delta Sct star 4CVn

V. S. Schmid, N. Themeßl, M. Breger +12

More than 40 years of ground-based photometric observations of the delta Sct star 4CVn revealed 18 independent oscillation frequencies, including radial as well as non-radial p-mod…

astro-ph.SR201422 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…