  We have conducted a study of debris disks around F stars in order to explore
correlations between rotation, stellar winds, and circumstellar disks. We
obtained new 24 micron photometry from Spitzer's Multiband Imaging Photometer
for Spitzer (MIPS) camera for a sample of 188 relatively nearby F dwarfs with
various rotation rates and optical colors, and combined it with archival MIPS
data for 66 more F stars, as well as Wide-field Infrared Survey Explorer (WISE)
data for the entire sample, plus 9 more F stars. Based on the objects' K_s-[24]
and [3.4]-[22] colors, we identify 22 stars in our sample as having 22 and/or
24 micron excesses above our detection limit, 13 of which are new discoveries.
Our overall disk detection rate is 22/263, or 8%, consistent with previous
determinations of disk fractions in the Solar neighborhood. While fast rotating
stars are expected to have strong winds capable of efficiently removing dust,
we find no correlation between rotational velocity and infrared excess.
Similarly, we find no significant difference in excess detection rate between
late-type F stars, which have convective surfaces, and early-type F stars,
which have fully radiative envelopes. However, the essentially unknown range of
ages in this sample may be washing out any effects relating rotation, winds,
and disks.
