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AKARI near-infrared spectroscopy of brown dwarfs

Published online by Cambridge University Press:  21 October 2010

Issei Yamamura ,
Takashi Tsuji ,
Toshihiko Tanabé  and
Tadashi Nakajima
Issei Yamamura
Affiliation:
Institute of Space and Astronautical Science, JAXA, Japan
Takashi Tsuji
Affiliation:
Institute of Astronomy, The University of Tokyo, Japan
Toshihiko Tanabé
Affiliation:
Institute of Astronomy, The University of Tokyo, Japan
Tadashi Nakajima
Affiliation:
National Astronomical Observatory, Japan
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Brown dwarfs (hereafter BDs) are of particular interest because of their extremely low-temperature atmospheres for comparison with atmospheres of giant planets. Aiming to obtain clues to understand the formation and disappearance of dust clouds and molecular abundances in BD photospheres, we conducted an observation programme of space-borne near-infrared spectroscopy of bright BDs with the Infrared Camera (IRC) on-board AKARI.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 545
Copyright
Copyright © International Astronomical Union 2010

References

Tsuji, T. 2002, ApJ 575, 264CrossRefGoogle Scholar
Tsuji, T. 2005, ApJ 621, 1033CrossRefGoogle Scholar