Abstract
We compare observations from 0.40 to 2.41um of the binary system CM Draconis with synthetic spectra computed using the stellar atmosphere code PHOENIX.
| Original language | English |
|---|---|
| Title of host publication | In: Brown Dwarfs and Extrasolar Planets - ASP Conf Series 134 |
| Publisher | Astronomical Society of the Pacific |
| Pages | 475-481 |
| ISBN (Print) | 1-886733-54-6 |
| Publication status | Published - 1998 |