Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 390, Issue 1, Pages L69-L72Publisher
OXFORD UNIV PRESS
DOI: 10.1111/j.1745-3933.2008.00541.x
Keywords
methods: numerical; galaxies: evolution; galaxies: haloes; galaxies: kinematics and dynamics; galaxies: structure
Categories
Funding
- [ANR-06-BLAN-0172]
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The Efstathiou, Lake and Negroponte (1982) criterion cannot distinguish bar stable from bar unstable discs and thus should not be used in semi-analytic galaxy formation simulations. I discuss the reasons for this, illustrate it with examples and point out shortcomings in the recipes used for spheroid formation. I propose an alternative, although much less straightforward, possibility.
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