TY  - GEN 
AU  - Pedersen, May G.
AU  - Chowdhury, Sowgata
AU  - Johnston, Cole
AU  - Bowman, Dominic M.
AU  - Aerts, Conny
AU  - Handler, Gerald
AU  - De Cat, Peter
AU  - Neiner, Coralie
AU  - David-Uraz, Alexandre
AU  - Buzasi, Derek
AU  - Tkatchenko, Andrew
AU  - Simón-Díaz, Sergio
AU  - Moravveji, Ehsan
AU  - Sikora, James
AU  - Mirouh, Giovanni Marcello
AU  - Lovekin, Catherine C.
AU  - Cantiello, Matteo
AU  - Daszyńska-Daszkiewicz, Jadwiga
AU  - Pigulski, Andrzej
AU  - Vanderspek, Roland K.
AU  - Ricker, George R.
PY  - 2019
UR  - https://hdl.handle.net/10481/111685
AB  - Uncertainties in stellar structure and evolution theory are largest for stars undergoing core convection on the main sequence. A powerful way to calibrate the free parameters used in the theory of stellar interiors is asteroseismology, which provides...
LA  - eng
PB  - IOP Publishing
KW  - Astrophysics - Solar and Stellar Astrophysics
KW  - asteroseismology
KW  - binaries: general
KW  - stars: evolution
KW  - stars: massive
KW  - stars: oscillations: including pulsations
KW  - stars: rotation
TI  - Diverse Variability of O and B Stars Revealed from 2-minute Cadence Light Curves in Sectors 1 and 2 of the TESS Mission: Selection of an Asteroseismic Sample
DO  - 10.3847/2041-8213/ab01e1
ER  -