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- W1522732287 abstract "Decompositions of the rotation curves of NGC2613, 3198, 6505, and 7184 are analysed. For these galaxies the radial velocity dispersions of the stars have been measured and their morphology is clearly discernible. If the parameters of the decompositions are chosen according to the `maximum' disk hypothesis, the Toomre Q stability parameter is systematically less than one and the multiplicities of the spiral arms as expected from density wave theory are inconsitent with the observed morphologies of the galaxies. The apparent Q<1 instability, in particular, is a strong argument against the `maximum' disk hypothesis." @default.
- W1522732287 created "2016-06-24" @default.
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- W1522732287 date "1998-12-02" @default.
- W1522732287 modified "2023-09-27" @default.
- W1522732287 title "NGC2613, 3198, 6503, 7184: Case studies against `maximum' disks" @default.
- W1522732287 hasPublicationYear "1998" @default.
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