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- Graz University of TechnologyAT3 papers
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- Bogolyubov Institute for Theoretical PhysicsUA1 paper
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- Max Planck Institute for AstrophysicsDE1 paper
- Sapienza University of RomeIT1 paper
- Simon Fraser UniversityCA1 paper
- Unité de Mathématiques Pures et AppliquéesFR1 paper
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astro-ph2005
Cosmological Simulations of Galaxy Formation I: Star Formation, Feedback, Resolution and Matching the Tully--Fisher Relation (among other things)
Fabio Governato, Greg Stinson, J. Wadsley +1
We used fully cosmological, high resolution N-body+SPH simulations to follow the formation of disk galaxies with a rotational velocity between 140 and 280 Km/sec in a Lambda CDM un…
astro-ph2004★ 7 cited
Disk Galaxy Rotation Curves in Triaxial CDM Halos
E. Hayashi, J. F. Navarro, A. Jenkins +7
We use N-body hydrodynamical simulations to study the structure of disks in triaxial potentials resembling CDM halos. Our analysis focuses on the accuracy of the dark mass distribu…