Double-barred starburst galaxies viewed by ISOCAM

Details Double-barred starburst galaxies viewed by ISOCAM Double-barred starburst galaxies viewed by ISOCAM

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.427..989w&link_type=abstract

The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427., p. 989

Computer Science

Isocam, Double-Barred Galaxies

Scientific paper

We present broad band 6.75 μm (LW2) and 15 μm (LW3) images that have been obtained with ISOCAM for two double-barred galaxies (NGC 1097 and NGC 4321) extracted from our global project WMFP15. These galaxies have both a large-scale stellar bar and a ~1 kpc scale nuclear bar surrounded by a circumnuclear ring. In the case of NGC 4321 both bars are aligned while they are misaligned in the case of NGC 1097. The comparison of their mid-infrared properties reveals that star formation is differently taking place in these objects.

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