We systematically searched the non-proprietary data in the Hobble Space Tel
escope (HST) Archive to identify low-redshift quasars that have been imaged
with the Wide Field Planetary Camera-2 (WFPC-2) but that have not yet been
presented in the literature. We identified five such objects. Since these
represent a significant increment to the number of WFPC-2. imaged quasars p
reviously presented in the Literature, we here present images of these obje
cts and a discussion of their properties.
Of the five objects, two are involved in spectacular ongoing gravitational
interactions. This brings the total number of quasars seen on WFPC-2 images
to be in such interactions to 11. A further two of the five quasars have c
lose companion objects (i.e. within 30 kpc) suggestive of a recent interact
ion. No evidence for an interaction can be seen on the fifth quasar.
All five host systems are brighter than L* in keeping with the results foun
d for other quasars imaged with WFPC-2. Three of the five quasars are at le
ast 2.5 mag brighter than L* and an among the brightest host galaxies image
d with WFPC-2. The results widen the derived difference in the mean absolut
e luminosity of the hosts of radio-quiet quasars compared with the hosts of
radio-loud quasars.