An HI shell-like structure associated with nova V458 Vulpeculae?
  We report the radio detection of a shell-like HI structure in proximity to,
and probably associated with, the nova V458 Vul. High spectral resolution
observation with the Giant Metrewave Radio Telescope has made it possible to
study the detailed kinematics of this broken and expanding shell. Unlike the
diffuse Galactic HI emission, this is a single velocity component emission with
significant clumping at ~ 0.5' scales. The observed narrow line width of ~ 5
km/s suggests that the shell consists of mostly cold gas. Assuming a distance
of 13 kpc to the system, as quoted in the literature, the estimated HI mass of
the nebula is about 25 M_sun. However, there are some indications that the
system is closer than 13 kpc. If there is a physical association of the HI
structure and the nova system, the asymmetric morphology and the off-centred
stellar system indicates past strong interaction of the mass loss in the
asymptotic giant branch phase with the surrounding interstellar medium. So far,
this is the second example, after GK Per, of a large HI structure associated
with a classical nova.
