Stellar halo constraints on simulated late-type galaxies
- 21 March 2004
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 349 (1) , 52-56
- https://doi.org/10.1111/j.1365-2966.2004.07464.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 32 references indexed in Scilit:
- Simulations of Galaxy Formation in a Λ Cold Dark Matter Universe. I. Dynamical and Photometric Properties of a Simulated Disk GalaxyThe Astrophysical Journal, 2003
- Three‐dimensional Simulations of the Chemical and Dynamical Evolution of the Galactic BulgeThe Astrophysical Journal, 2003
- Galactic Halo Stars in Phase Space: A Hint of Satellite Accretion?The Astrophysical Journal, 2003
- Can Photoionization Squelching Resolve the Substructure Crisis?The Astrophysical Journal, 2002
- Star Formation, Supernova Feedback, and the Angular Momentum Problem in Numerical Cold Dark Matter Cosmogony: Halfway There?The Astrophysical Journal, 2001
- Implementing Feedback in Simulations of Galaxy Formation: A Survey of MethodsThe Astrophysical Journal, 2000
- Dark Halo and Disk Galaxy Scaling Laws in Hierarchical UniversesThe Astrophysical Journal, 2000
- A Unified Scaling Law in Spiral GalaxiesThe Astrophysical Journal, 2000
- BR photometry of the halo of M31The Astronomical Journal, 1994
- Subdwarf Studies. III. The Halo Metallicity DistributionThe Astronomical Journal, 1991