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- W1967322575 abstract "Axisymmetric dynamical models are constructed for the E3 galaxy M32 to interpret high spatial resolution stellar kinematical data obtained with the Hubble Space Telescope (HST). Models are studied with two-integral, f(E, Lz), phase-space distribution functions and with fully general three-integral distribution functions. The latter are built using an extension of Schwarzschild's approach: individual orbits in the axisymmetric potential are calculated numerically, and populated using nonnegative least-squares fitting so as to reproduce all available kinematical data, including line-of-sight velocity profile shapes. The details of this method are described in companion papers by Rix et al. and Cretton et al." @default.
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- W1967322575 date "1998-02-01" @default.
- W1967322575 modified "2023-10-18" @default.
- W1967322575 title "Improved Evidence for a Black Hole in M32 from<i>HST</i>/FOS Spectra. II. Axisymmetric Dynamical Models" @default.
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- W1967322575 doi "https://doi.org/10.1086/305147" @default.
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