An infrared spectral sequence into the brown dwarf regime

Details An infrared spectral sequence into the brown dwarf regime An infrared spectral sequence into the brown dwarf regime

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...196.0301j&link_type=abstract

American Astronomical Society, 196th AAS Meeting, #03.01; Bulletin of the American Astronomical Society, Vol. 32, p.676

Astronomy and Astrophysics

Astronomy

Scientific paper

A spectral sequence from mid-type M dwarfs into the brown dwarf regime is presented. These spectra cover the wavelength range 0.8 to 2.4 microns and measure the peak of the spectral energy distribution for these extremely red objects. The spectra were taken with the Hubble Space Telescope and represent an infrared spectra of M dwarfs and brown dwarfs which are free from the problems of correcting for the terrestial atmospheric absorption.

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