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 |