  We present CO(1-0) and CO(2-1) line emission maps of the barred spiral active
galaxy HE1029-1831 (z=0.0403) obtained with the IRAM Plateau de Bure
Interferometer (PdBI) and in part by the Berkeley-Illinois-Maryland Association
(BIMA) observatory. The CO emission is well associated with the optical bar and
extended along it. The FWHM of the CO emission is estimated to be ~(6+-2)kpc.
The CO emission shows a strong velocity gradient along the minor axis of the
bar (PA=90degree). The molecular gas mass is estimated to be ~1.2x10^(10)Msun
which indicates a very gas rich host galaxy. Most of the molecular gas appears
to be subthermally excited and cold but we also find weak evidence for a warmer
and/or denser gas component at the southern part of the bar emission, about
\~4kpc from the galactic nucleus.
