Atmospheric Model of a dM Star with Planets
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.
- Publication:
-
Living Together: Planets, Host Stars and Binaries
- Pub Date:
- July 2015
- Bibcode:
- 2015ASPC..496..344V