AKARI near-infrared spectroscopy of brown dwarfs

Details AKARI near-infrared spectroscopy of brown dwarfs AKARI near-infrared spectroscopy of brown dwarfs

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15..545y&link_type=abstract

Highlights of Astronomy, Volume 15, p. 545-545

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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