Abstract: We present $ H$ - band scattered light imaging of
a bright debris disk around the A0 star HD 36546 obtained from the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system with data recorded by the HiCIAO camera using the vector vortex coronagraph.
Massive numbers of comets may even produce
the bright debris disks seen around other stars.
In 2010 we began a near - infrared (NIR) spectral survey of
bright debris disks with reported IRAS excesses and optically resolved disks.
Not exact matches
The observed 100 um fluxes from delta Pav, HR 8501, and 51 Peg agree with the predicted photospheric fluxes, excluding
debris disks brighter than Ldust / Lstar ~ 5 x 10 ^ -7 (1 sigma level) around those stars.