Phoenix High Resolution Observations of Ultracool Dwarfs.

Details Phoenix High Resolution Observations of Ultracool Dwarfs. Phoenix High Resolution Observations of Ultracool Dwarfs.

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.1103h&link_type=abstract

American Astronomical Society Meeting 205, #11.03; Bulletin of the American Astronomical Society, Vol. 36, p.1352

Astronomy and Astrophysics

Astronomy

Scientific paper

High resolution K-band spectra of three ultracool dwarfs of spectral types M8, L4.5, and L8 were obtained from the Phoenix spectrograph on the Gemini South 8-meter telescope. These observations yield the effective temperatures and surface gravities of these ultracool objects. Their spectral energy distributions are compared to brown dwarf model atmospheres with and without atmospheric dust.

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