First detection of main-sequence stars at 3 mm wavelength


Context. The precise mechanisms that provide the non-radiative energy for heating the chromosphere and the corona of the Sun and those of other stars constitute an active field of research. By studying stellar chromospheres one aims at identifying the relevant physical processes. Defining the permittable extent of the parameter space can also serve as a… (More)

3 Figures and Tables


  • Presentations referencing similar topics