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A Near-Infrared Spectral Sequence of Late M, L, and T Dwarfs

Published online by Cambridge University Press:  26 May 2016

Michael C. Cushing ,
John T. Rayner  and
William D. Vacca
Michael C. Cushing
Affiliation:
Institute for Astronomy, University of Hawai'i, 2680 Woodlawn Drive, Honolulu HI, 96822
John T. Rayner
Affiliation:
Institute for Astronomy, University of Hawai'i, 2680 Woodlawn Drive, Honolulu HI, 96822
William D. Vacca
Affiliation:
Max-Planck-Institute für Extraterrestrische Physik, Postfach 1312, D-85741 Garching, Germany

Abstract

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We present the initial results of a medium resolution, 0.8 to 4.2 μm spectroscopic survey of M, L, and T dwarfs. We have identified the most prominent molecular and atomic absorption features found in the spectra of these late-type dwarfs. We have also compared the spectra to a laboratory FeH emission spectrum and identified nearly 100 features common to the FeH spectrum and the dwarf spectra from 0.99 to 1.8 μm.

Type
Part 7. Atmospheres and Internal Structure
Information
Symposium - International Astronomical Union , Volume 211: Brown Dwarfs , 2003 , pp. 389 - 392
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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