Can bars be destroyed by a central mass concentration?-- I. Simulations
Open Access
- 21 October 2005
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 363 (2) , 496-508
- https://doi.org/10.1111/j.1365-2966.2005.09445.x
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This publication has 56 references indexed in Scilit:
- On the nature of bulges in general and of box/peanut bulges in particular: input fromN-body simulationsMonthly Notices of the Royal Astronomical Society, 2005
- Dynamical Evolution of Barred GalaxiesCelestial Mechanics and Dynamical Astronomy, 2005
- What determines the strength and the slowdown rate of bars?Monthly Notices of the Royal Astronomical Society, 2003
- Bar-Halo Interaction and Bar GrowthThe Astrophysical Journal, 2002
- Morphology, photometry and kinematics of N-body bars — I. Three models with different halo central concentrationsMonthly Notices of the Royal Astronomical Society, 2002
- Optimal softening for force calculations in collisionless N-body simulationsMonthly Notices of the Royal Astronomical Society, 2000
- The existence and shapes of dust lanes in galactic barsMonthly Notices of the Royal Astronomical Society, 1992
- Morphology of bar orbitsMonthly Notices of the Royal Astronomical Society, 1992
- A hierarchical O(N log N) force-calculation algorithmNature, 1986
- Star distribution around a massive black hole in a globular clusterThe Astrophysical Journal, 1976