2 citations · 2 across the 2 of their papers we have counts for
2 papers
astro-ph2003
Star formation and turbulent dissipation in models of disk galaxy evolution
V. Avila-Reese, C. Firmani, E. Vazquez-Semadeni
The kinetic energy dissipation rate in the turbulent ISM of disk galaxies is a key ingredient in galaxy evolution models since it determines the effectiveness of large-scale star f…
astro-ph2003★ 2 cited
Physical processes behind the morphological Hubble sequence
C. Firmani, V. Avila-Reese
The study of formation and evolution of galaxies is reviewed, making emphasis on the physical factors which are important to understand the origin of the galaxy Hubble sequence. We…