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The Eclipsing Binary System CM Draconis
(Astronomical Society of the Pacific, 1998)
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.
A Comparison of the Infrared Spectra of Two Very Late-type M Dwarfs with Different Gravities
(Astronomical Society of the Pacific, 1998)
We present observations obtained during the commissioning of the upgraded Cooled Grating Spectrometer 4 on the UK Infrared Telescope on Mauna Kea, of the very low-mass objects TVLM 513-46546 and Gl 569B. Spectra were taken ...
Water and titanium oxide in late-type M dwarfs
(Astronomical Society of the Pacific, 1996)
Despite the identification of brown dwarf candidates the lack of understanding of M dwarfs has meant that it has not been possible to unambiguously distinguish these candidates from cool M dwarfs. Unlike hotter stars their ...