ASPCS
 
Back to Volume
Paper: Atmospheric Model of a dM Star with Planets
Volume: 496, Living Together: Planets, Host Stars and Binaries
Page: 344
Authors: Vieytes, M. C.; Fontenla, J. M.; Buccino, A. P.; Mauas, P. J. D.
Abstract: We present our first attempt to model the atmosphere of GJ 876, a weakly active dM star with planets. We built a photospheric and chromospheric full NLTE model using the Solar Radiation Physical Modeling code (SRPM), which was upgraded to take into account molecular features that become important in the spectrum of a cooler star than the Sun.
Back to Volume