The Stellar Velocity Dispersion in the Inner 1.3 Disk Scale Lengths of the Irregular Galaxy NGC 4449

We present measurements of the stellar velocity dispersion in the inner 1ʹ radius (1.3 disk scale lengths) of the irregular galaxy NGC 4449 determined from longslit absorption-line spectra. The average observed dispersion is 29 ± 2 km s-1, the same as predicted from NGC 4449ʹs luminosity. No significant rotation in the stars is detected. If we assume a maximum rotation speed of the stars from the model determined from the gas kinematics of Hunter et al., the ratio Vmax/(sigma)z measured globally is 3. This ratio is comparable to values measured in spiral galaxies and implies that the stellar disk in NGC 4449 is kinematically relatively cold. The intrinsic minor-to-major axis ratio (b/a)0 is predicted to be in the range 0.3-0.6, similar to values derived from the distribution of observed b/a of Im galaxies. However, V/(sigma)z measured locally is 0.5-1.1, and so the circular velocity of NGC 4449 is comparable to or less than the velocity of the stars within the central 1.3 disk scale lengths of the galaxy.