NASA NTRS · 20060040766
Exozodiacal Disk Detection Potential with the Keck Interferometer
Abstract
If 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.
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Serabyn, E., Colavita, M., Beichman, C.. 1999-04-25. Exozodiacal Disk Detection Potential with the Keck Interferometer. https://ntrs.nasa.gov/citations/20060040766
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