Why there are no elliptical galaxies more flattened than E7: Thirty years later
Elliptical galaxies are modeled as homeoidally striated Jacobi ellipsoids (Caimmi and Marmo 2005) where the peculiar velocity distribution is anisotropic, or equivalently as their adjoint configurations i.e. classical Jacobi ellipsoids of equal mass and axes, in real or imaginary rotation (Caimmi 20...
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| Aineistotyyppi: | Artikkeli |
| Kieli: | English |
| Julkaistu: |
Astronomical Observatory, Department of Astronomy, Belgrade
2006-01-01
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| Sarja: | Serbian Astronomical Journal |
| Aiheet: | |
| Linkit: | http://www.doiserbia.nb.rs/img/doi/1450-698X/2006/1450-698X0673013C.pdf |