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Keck II Mid-Infrared Imaging of the Young Stellar Object WL16WL16 is unique among the members of the young, forming star cluster embedded in the nearby p Oph cloud core in exhibiting an extended, high surface brightness disk in the emission features originating from solid-state aromatic hydrocarbons.
Document ID
20060040572
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/16901
Authors
Ressler, M.
Barsony, M.
Date Acquired
August 23, 2013
Publication Date
February 1, 1999
Publication Information
Publication: Astrophysical Journal Letters
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
Circumstellar matter dust disk mid-infrared very small grains formation
pre-main-sequence stars star formation

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