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Discovery of a faint Field Methane Brown Dwarf from ES0 NTT and VLT observations

J. G. Cuby, P. Saracco, A. F. M. Moorwood, S. D'Odorico, C. Lidman, F. Comeron, J. Spyromilio

astro-pharXiv:astro-ph/9907028

Abstract

We report the discovery of an isolated brown dwarf with similar properties to the binary object Gliese 229B and to the newly discovered field brown dwarf SDSS 1624+00. Although exhibiting similar colors, its magnitude of ~20.5 is about 6 and 5 magnitudes fainter than Gliese 229B and SDSS 1624+00 respectively. This is the third methane brown dwarf reported to date, the second isolated one in the field and by far the most distant at ~ 100 pc. Its IR spectrum, although at low S/N given the faintness of the object, is remarkably similar to those of the 2 other methane brown dwarfs.

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