Structure of the MIR Emission in the Circum-Nuclear Regions of Active and/or Starburst Galaxies

Details Structure of the MIR Emission in the Circum-Nuclear Regions of Active and/or Starburst Galaxies Structure of the MIR Emission in the Circum-Nuclear Regions of Active and/or Starburst Galaxies

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.460..523w&link_type=abstract

The Promise of the Herschel Space Observatory. Eds. G.L. Pilbratt, J. Cernicharo, A.M. Heras, T. Prusti, & R. Harris. ESA-SP 460

Computer Science

Galaxies: Nuclei, Galaxies: Circumnuclear Regions, Galaxies: Star Formation

Scientific paper

We present broad band 7 micron (LW2) and 15 micron (LW3) images that
have been obtained with ISOCAM for a sample of ten barred galaxies. The
comparison of their mid-infrared properties reveals that star formation
is differently taking place in these objects.

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