202 citations · 1.8k across the 28 of their papers we have counts for
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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…
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…
KIC 10526294: a slowly rotating B star with rotationally split, quasi-equally spaced gravity modes
P. I. Pápics, E. Moravveji, C. Aerts +4
Massive stars are important for the chemical enrichment of the universe. Since internal mixing processes influence their lives, it is very important to place constraints on the cor…
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…
Separated Fringe Packet Observations with the CHARA Array II: Andromeda, HD 178911, and ξ Cephei
Christopher D. Farrington, Theo A. ten Brummelaar, Brian D. Mason +7
When observed with optical long-baseline interferometers (OLBI), components of a binary star which are sufficiently separated produce their own interferometric fringe packets; thes…
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…