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Exozodiacal Disk Detection Potential with the Keck InterferometerIf the dust content of nearby solar system is comparable to, or larger than, that of our own zodiacal disk, the thermal emission from exozodiacal disks will significantly outshine planetary companions to nearby stars.
Document ID
20060040766
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
hdl:2014/17817
Authors
Serabyn, E.
Colavita, M.
Beichman, C.
Date Acquired
August 23, 2013
Publication Date
April 25, 1999
Subject Category
Instrumentation And Photography
Distribution Limits
Public
Copyright
Other
Keywords
exozodiacal disk Keck interferometer MIR Keck nulling

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