Where are the M Dwarf Exo-Zodiacal Disks?

Details Where are the M Dwarf Exo-Zodiacal Disks? Where are the M Dwarf Exo-Zodiacal Disks?

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..357..127p&link_type=abstract

The Spitzer Space Telescope: New Views of the Cosmos ASP Conference Series, Volume 357, proceedings of the conference held 9-12

Astronomy and Astrophysics

Astronomy

Scientific paper

We present 11.7μm observations of nine late-type dwarfs obtained at the Keck I telescope. Our targets were selected for their youth or apparent IRAS 12μm excess. For all sources, excess infrared emission is not detected. We find that stellar wind drag can dominate the circumstellar grain removal and plausibly explain the dearth of M Dwarf systems with infrared excesses.

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