  This paper is primarily a study of the effect of a bar on the neutral
hydrogen (HI) content of starburst and Seyfert galaxies. We also make
comparisons with a sample of ``normal'' galaxies and investigate how well
starburst and Seyfert galaxies follow the fundamental scaling Tully-Fisher (TF)
relation defined for normal galaxies. 111 Markarian (Mrk) IRAS galaxies were
observed at the Nancay radiotelescope. These measurements are complemented by
data from the literature to form a sample of 105 unbarred and 113 barred Mrk
IRAS galaxies. Barred galaxies have lower total and bias-corrected HI masses
than unbarred galaxies, and this is true for both Mrk IRAS and normal galaxies.
This robust result suggests that bars funnel the HI gas toward the center of
the galaxy where it becomes molecular before forming new stars. The Mrk IRAS
galaxies have higher bias-corrected HI masses than normal galaxies. They also
show significant departures from the TF relation, both in the B and K bands.
The most deviant points from the TF relation tend to have a strong far-infrared
luminosity and a low oxygen abundance. These results suggest that a fraction of
our Mrk IRAS galaxies are still in the process of formation, and that their
neutral HI gas, partly of external origin, has not yet reached a stationary
state.
