Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...267..109b&link_type=abstract
Astrophysical Journal, Part 1, vol. 267, Apr. 1, 1983, p. 109-118.
Astronomy and Astrophysics
Astrophysics
2
Density Wave Model, Galactic Structure, Hydrodynamics, One Dimensional Flow, Shock Fronts, Spiral Galaxies, Transition Flow, Astronomical Models, Disk Galaxies, Flow Velocity, Gas Flow, Gas Heating, Gravitational Fields, Sine Waves
Scientific paper
The problem of one-dimensional gas flow through a sinusoidal gravitational potential with a series of equally spaced shock fronts is considered. For time-independent and spatially periodic flows, an integral equation relates the flow velocity to the gravitational potential and source functions of energy and momentum densities. It is suggested that this problem simulates some of the dynamical effects of the azimuthal flow on a parcel of gas at a fixed radius in a galactic disk that supports a spiral density wave structure. It omits the radial motions. In this context, a typical azimuthal velocity across a spiral arm is specified and the resultant source functions are obtained. The implications of this calculation suggest heating of the gaseous disk by O and B stars behind the shock front, and subsequent interarm cooling is a plausible mechanism for maintaining the periodic cycling of the gaseous component of the galactic disk.
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