The line-of-sight velocity distributions of simulated merger remnants
Open Access
- 1 August 2000
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 316 (2), 315-325
- https://doi.org/10.1046/j.1365-8711.2000.03475.x
Abstract
No abstract availableThis publication has 31 references indexed in Scilit:
- Orthogonal Rotating Gaseous Disks near the Nucleus of NGC 253The Astrophysical Journal, 1996
- Structure of Merger Remnants. V. KinematicsThe Astrophysical Journal, 1996
- Formation of Massive Counterrotating Disks in Spiral GalaxiesThe Astrophysical Journal, 1996
- The Post-Merger Elliptical NGC 1700: Stellar Kinematic Fields to Four Effective RadiiThe Astronomical Journal, 1996
- Structure of merger remnants. 4: Isophotal shapesThe Astrophysical Journal, 1994
- Origin of kinematic subsystems in elliptical galaxiesNature, 1991
- Counter-rotation in dust-lane ellipticals and the implications for accretion events in galaxiesNature, 1988
- Recognizing merger remnants among normal elliptical galaxies NGC 5813The Astrophysical Journal, 1984
- Simulations of sinking satellitesThe Astrophysical Journal, 1983
- The Dynamics of the Interstellar Medium. III. Galactic Distribution.The Astrophysical Journal, 1942