What Makes the Family of Barred Disc Galaxies so Rich: Damping Stellar Bars in Spinning Haloes
Clayton H. Heller
Part of the Physical Sciences and Mathematics Commons
Works by Isaac Shlosman in Physical Sciences and Mathematics
2020
What Makes the Family of Barred Disc Galaxies so Rich: Damping Stellar Bars in Spinning Haloes
Clayton H. Heller
Dark Matter Halos and Evolution of Bars in Disk Galaxies: Varying Gas Fraction and Gas Spatial Resolution
Clayton H. Heller
Dissecting Galaxy Formation. I. Comparison Between Pure Dark Matter and Baryonic Models
Clayton H. Heller
Structure Formation Inside Triaxial Dark Matter Halos: Galactic Disks, Bulges, and Bars
Clayton H. Heller
Dissecting Galaxy Formation. II. Comparing Substructure in Pure Dark Matter and Baryonic Models
Clayton H. Heller
Dark Matter Halos and Evolution of Bars in Disk Galaxies: Collisionless Models Revisited
Clayton H. Heller
Evolution of Stellar Bars in Live Axisymmetric Halos: Recurrent Buckling and Secular Growth
Clayton H. Heller
2014
2010
2009
2008
2007
2006
2002
2001
Double Bars in Disk Galaxies: Dynamical Decoupling of Non-Self-gravitating Gaseous Bars
Clayton H. Heller