Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..504n&link_type=abstract
(Pis'ma v Astronomicheskii Zhurnal, vol. 12, July 1986, p. 504-521) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, July-Aug
Astronomy and Astrophysics
Astronomy
8
Galactic Rotation, Spiral Galaxies, Vortices, Angular Velocity, Density Wave Model, Galactic Structure, Particle Motion, Radial Velocity, Shallow Water, Simulation
Scientific paper
A rotating, two-zone, shallow-water laboratory simulation, designed to illustrate how spiral structure might be generated in galaxies whose rotation curve shows a jump in velocity, discloses anticyclonic, banana-shaped vortices at points of minimum surface density between successive spiral arms. Fluid particles trapped in these 'whorls' will enter and flow along the arms, achieving substantial radial velocities near the corotation circle (the rotation-curve discontinuity). This behavior, interpreted theoretically, provides new insight into the relative motion of the spiral arms and the gas in a galaxy disk. A self-consistent spiral/whorl structure emerges even if the peripheral zone rotates so fast that the Rossby-Obukhov radius is an order of magntitude shorter than the arms. The model results are compared with observations of NGC 1566. In some SB galaxies the bar phenomenon may be an artifact of spiral/whorl structure in the gaseous disk. If a rotating spiral galaxy interacts with a companion orbiting in the opposite direction, spiral arms can be produced which intrinsically lead: the pattern would rotate, tips forward, opposite to the rotation in the galaxy's interior.
Fridman Alexei M.
Nezlin Michael V.
Polyachenko Valerij L.
Snezhkin E. N.
Trubnikov A. S.
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