Back to the top of Aschig's Universe

• Contents
• List of Tables
• List of Figures
• Overview
  • Introduction
  • Present Work
  • Future Possibilities
• Observations: the raw material
  • The sample
  • Observations
  • Calibration
  • Control Sample
• Brightness distribution
  • Introduction
  • The radial profile
  • The different components
  • Decomposing the profile
  • Consistency checks
  • 2D distribution
  • Summary
• Scale lengths at different wavelengths
  • Results of profile fits
  • Color gradients
  • Extrapolated profiles
  • Conclusions
• Radio galaxies with disks
  • Disky galaxies
  • Morphological Signatures of disks
  • Discussion
• Dusty galaxies
  • Introduction
  • Detection techniques
  • Dust lane galaxies
  • Discussion and conclusions
• Radio structure: using a different eye
  • Introduction
  • Optical-radio correlations
  • Induced star formation
  • Conclusions
• Ages: how recent is the blue
  • Introduction
  • The existing picture
  • Synthetic spectra
  • Age of the most recent starburst
• Conclusions
  • The emerging picture
  • The work goes on
• Morphological processing
  • Dilation and erosion
  • Opening and closing
  • Gradient
• Individual objects
• References