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- W160147173 abstract "A detailed morphological and kinematical study of the close pair of galaxies UGC 9922 is presented. The larger galaxy, which resembles a perturbed bar with three knots, shows peculiar internal motions. The ionized gas is in differential rotation, with a maximum velocity of about 120 km/s, and a very low gradient near the center, possibly due to streaming motions. The stars follow the gas in the innermost regions, rotate in the opposite sense between 0.7 and 2.2 kpc, and rotate in the same sense as the gas, but much faster (maximum rotation velocity: 180 km/s) in the outer regions. These kinematical peculiarities may be accounted for by a ring of counter-rotating stars, presumably due to a former companion spiralling toward the center of the galaxy in a retrograde orbit, and by an outer warp of the gaseous component, due to the present companion" @default.
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- W160147173 date "1991-12-01" @default.
- W160147173 modified "2023-09-24" @default.
- W160147173 title "Counter-rotation in the interacting starburst galaxies UGC 9922" @default.
- W160147173 hasPublicationYear "1991" @default.
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