Images of neutral hydrogen 21 cm absorption and radio continuum emission at
1.4 GHz from Mrk 273 were made using the Very Long Baseline Array and Very
Large Array. These images reveal a gas disk associated with the northern n
uclear region with a diameter 0."5 (370 pc) at an inclination angle of 53 d
egrees. The radio continuum emission is composed of a diffuse component plu
s a number of compact sources. This morphology resembles those of nearby, l
ower luminosity starburst galaxies. These images provide strong support for
the hypothesis that the luminosity of the northern source is dominated by
an extreme compact starburst. The H I 21 cm absorption shows an east-west g
radient in velocity of 450 km s(-1) across 0."3 (220 pc), which implies an
enclosed mass of 2 x 10(9) M-circle dot, comparable to the molecular gas ma
ss. The brightest of the compact sources may indicate radio emission from a
n active nucleus, but this source contributes only 3.8% to the total flux d
ensity of the northern nuclear regions. The H I 21 cm absorption toward the
southeast radio nucleus suggests infall at 200 km s(-1) on scales less tha
n or equal to 40 pc, and the southwest near-LR nucleus is not detected in h
igh-resolution radio continuum images.