Extended coronal emission lines in active galactic nuclei
VLT and NTT spectra are used to examine the nuclear and extended coronal line emission in a sample of well-known Seyfert 1 and 2 galaxies. The excellent spatial resolution obtained with VLT allowed us to map [Si VI] 1.963μm and [Si VII] 2.48μm on scales of up to 20 pc. Coronal line emission, extended to distances of ˜102 pc, is detected in some of
Rodríguez-Ardila, Alberto et al.
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11
2004