ISOCAM-CVF 5-12 mum Spectroscopy of Ultraluminous Infrared Galaxies
(2001)
CO-Observations of Post-Starburst Galaxies
Chapter in The Evolution of Galaxies, Springer Nature (2001) 95-95
CO-observations of post-starburst galaxies
ASTROPHYSICS AND SPACE SCIENCE 277 (2001) 95-95
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