MAMSIE Board Meeting I • Leuven, 31 January 2017, 10h30-12h30 followed by a joint lunch, Van Hoof seminar room, Institute of Astronomy, KU Leuven • In attendance: Profs J. Christensen-Dalsgaard, T. Rogers, S. Mathis, C. Aerts; MAMSIE team members: A. Tkachenko, C. Johnston, E. Vermeyen, D. Bowman (B. Buysschaert and M. G. Pedersen at work abroad); other Leuven team members: E. Moravveji, P. Pápics, T. Van Reeth, S. Sekaran, V. Schmid
Application to single & binary stars with mass between 3 and 30 solar masses, magnetic and non-magnetic, slow and fast rotators… meanwhile broadened to: single & binary stars born with a convective core… + TESS CVZ stars with low & high metallicity
MAMSIE employees: 4 PhD students, 2 postdocs Bram Buysschaert (co-tutelle Meudon-Leuven), May Gade Pedersen, Cole Johnston, Enya Vermeyen Andrew Tkachenko (2016), Dominic Bowman (2017,2018) 7-9 September 2016 kick-off with team of Prof. Tami Rogers: postdoc Philipp Edelmann PhD student Rathish Ratnasingam
Application to single & binary stars with Bram: magnetism mass between 3 and 30 solar masses, magnetic May Cole and non-magnetic, slow and fast rotators… Enya meanwhile broadened to: Dominic TBD: single & binary Andrew 2018 stars born with a Conny convective core… + TESS CVZ stars with low & high TBD: 2018 metallicity
other Leuven team members in asteroseismology: + ERC runner up FWO project led by Andrew Tkachenko: 1 PhD student Sanjay Sekaran (Nov. 2016) scaling relations deduced for heat-driven pulsators and solar-like pulsators in binaries postdocs Ehsan Moravveji (MC until June 2017), + Péter Pápics (FWO until Sept. 2017), & (soon-to-be) Timothy Van Reeth (until Sept. 2017)
PhD research May Gade Pedersen: forward seismic modelling of single B star pulsators with period spacing patterns Started June 2016: participation in MESA summer school getting familiar with MESA/GYRE focus on near-core mixing
PhD research May Gade Pedersen: aim to improve forward seismic modelling of two Kepler SPBs with lack of near-core mixing Moravveji et al. (2015, 2016)
Pápics et al. (2017)
Pápics et al. (2017)
Pápics et al. (2017)
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