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
The European Large Area ISO Survey - IV. The preliminary 90-渭m luminosity function
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 322:2 (2001) 262-268
The European Large-Area Infrared Space Observatory Survey V:: a BeppoSax hard X-ray survey of the S1 region
ASTROPHYSICAL JOURNAL 554:1 (2001) 18-26
The extended counterpart of submm source Lockman 850.1
ASTRONOMY & ASTROPHYSICS 378:1 (2001) 70-75