The following document lists the file abstract/DVBUREN_PSR_CAM.abs
from catalogue VI/111.
A plain copy of the file
(without headers/trailers) may be downloaded.
At least one pulsar, PSR1257+12 has planets. Their origin is mysterious, but some theories hold that they were formed in a debris disk after the supernova explosion. Such a debris disk is expected to be detectable by ISO, and we propose here a small survey of young pulsars using CAM. We have previously examined the IRAS data and found 13 pulsars at the positions of PSC sources, but this number is consistent with chance coincidence. We want now to go 100 times deeper with a small sample of young pulsars, imaging in 4 ISOCAM bands to get colors.