Analysis of the peculiar velocities of neutral hydrogen H I in the spiral galaxy M 81

Astronomy and Astrophysics – Astronomy

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Flow Velocity, Gas Dynamics, Hydrogen Clouds, Interstellar Gas, Spiral Galaxies, Density Wave Model, Radial Velocity, Velocity Distribution

Scientific paper

Allowance for noncircular gas motion in the analysis of the M 81 velocity field made it possible to identify the radial motion of the gas toward the center and the spiral field of the peculiar velocities. The latter can be described by a logarithmic spiral with a pitch angle of 8.2 + or - 1 deg. The parameters of the spiral density wave were determined under the assumption that the spiral field of the peculiar velocities is wavelike in nature.

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