output
19912026
most citedStarburst99: Synthesis Models for Galaxies with Active Star Formation

4k citations

Showing 2005 · astro-phShow all

14 papers · 2 filters

astro-ph2005★ 50 cited

The 21 Centimeter Background from the Cosmic Dark Ages: Minihalos and the Intergalactic Medium before Reionization

Paul R. Shapiro, Kyungjin Ahn, Marcelo A. Alvarez +3

The H atoms inside minihalos (i.e. halos with virial temperatures T_vir < 10^4 K, in the mass range roughly from 10^4 M_sun to 10^8 M_sun) during the cosmic dark ages in a LambdaCD…

astro-ph2005★ 4 cited

Gas Rich Mergers in Disk Formation

Chris B. Brook, Vincent Veilleux, Daisuke Kawata +2

In order to explain disk galaxy formation within the hierarchical structure formation, it seems that gas rich mergers must play an important role. We review here our previous studi…

astro-ph2005★ 3 cited

Understanding the Equilibrium Structure of CDM Halos

Paul R. Shapiro, Kyungjin Ahn, Marcelo Alvarez +2

N-body simulations find a universal structure for the halos which result from the nonlinear growth of Gaussian-random-noise density fluctuations in the CDM universe. This talk summ…

astro-ph2005★ 18 cited

HI Detection in two Dwarf S0 Galaxies in Nearby Groups: ESO384-016 and NGC 59

Sylvie F. Beaulieu, Kenneth C. Freeman, Claude Carignan +2

An \hi survey of 10 dE/dS0 galaxies in the nearby Sculptor and Centaurus A groups was made using the Australia Telescope Compact Array (ATCA). The observed galaxies have accurate d…

astro-ph2005★ 8 cited

The 21-cm Background from the Cosmic Dark Ages: Minihalos and the Intergalactic Medium before Reionization

Kyungjin Ahn, Paul R. Shapiro, Marcelo A. Alvarez +3

The H atoms inside minihalos (i.e. halos with virial temperatures T_vir < 10^4 K, in the mass range roughly from 10^4 M_sun to 10^8 M_sun) during the cosmic dark ages in a LCDM uni…

astro-ph2005

The Evolving Structure of Galactic Disks

Hugo Martel, Chris Brook, Sean McGee +2

Observations suggest that the structural parameters of disk galaxies have not changed greatly since redshift 1. We examine whether these observations are consistent with a cosmolog…