Galaxy mapping with the SAURON integral-field spectrograph: The star formation history of NGC 4365
ASTROPHYSICAL JOURNAL 548:1 (2001) L33-L36
Gas flow and star formation in the "Antennae" galaxies
ASTR SOC P 240 (2001) 214-215
Abstract:
The prominent interacting galaxy pair NGC4038/9 contains many active star-forming regions and is continuously forming new star clusters. We present a self-consistent N-body model for this system which includes an SPH gas component. The model qualitatively explains tile apparent concentration of gas in the so-called overlap region between the two nuclei as a bridge of gas connecting the two galaxies. Projected on the sky, the bridge appears as a dense spot of gas. We discuss some implications for the evolution of ultra-luminous infrared galaxies.ISOCAM-CVF 5-12 micron spectroscopy of ultraluminous infrared galaxies
ASTROPHYSICAL JOURNAL 552:2 (2001) 527-543
Line-of-sight velocity distributions of low-luminosity elliptical galaxies
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 326:2 (2001) 473-489
Near-Infrared Integral Field Spectroscopy of Damped Lyman- Systems
Chapter in Mining the Sky, Springer Nature (2001) 214-217