activity
19992005
most citedHalpha rotation curves: the soft core question

143 citations · 221 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2005★ 76 cited

The clustering of the luminosities of optical afterglows of long Gamma Ray Bursts

M. Nardini, G. Ghisellini, G. Ghirlanda +3

We studied the optical afterglows of the 24 pre-Swift Gamma-Ray Bursts with known spectroscopic redshift and published estimates of the optical extinction in the source frame. We f…

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…

astro-ph2002

The shape of rotation curves: models vs. observations

V. Avila-Reese, C. Firmani, J. Zavala

We discuss the shape and decomposition of rotation curves (RCs) of galaxies formed within growing cold dark matter halos. The outer RC shape correlates mainly with the surface brig…

astro-ph2002★ 143 cited

Halpha rotation curves: the soft core question

D. Marchesini, E. D'Onghia, G. Chincarini +4

We present high resolution Halpha rotation curves of 4 late-type dwarf galaxies and 2 low surface brightness galaxies (LSB) for which accurate HI rotation curves are available from…

astro-ph1999

Structure, dynamics and evolution of disk galaxies in a hierarchical formation scenario

C. Firmani, V. Avila-Reese

Using galaxy evolutionary models in a hierarchical formation scenario, we predict the structure, dynamics and evolution of disk galaxies in a LCDM universe. Our models include star…