10.25405/data.ncl.9192326.v1 Philipp Edelmann Philipp Edelmann Rogers, Tamara M. Tamara M. Rogers Ratnasingam, R. P. R. P. Ratnasingam Dominic Bowman Dominic Bowman Pedersen, May Gade May Gade Pedersen Convection and Internal Gravity Waves in a Main-Sequence Star Newcastle University 2019 internal gravity waves hydrodynamics main-sequence star convection Astrophysics Stellar Astronomy 2019-07-31 08:43:10 Media https://data.ncl.ac.uk/articles/media/Convection_and_Internal_Gravity_Waves_in_a_Main-Sequence_Star/9192326 <div>This shows a three-dimensional hydrodynamics simulation of a main-sequence star of three solar masses. The star has a convection zone at its core and a radiative envelope. Internal gravity waves are being excited at the interface between these two zones and propagate outward. The colour scale represents the temperature deviations from the horizontal mean.</div><div><br></div><div><br></div>