Near infrared surface photometry of NGC 1068.
NGC 1068 has been observed at the near infrared bands J, H, K, L. Near infrared scans of NGC 1068 with 20 and 5 arcsec apertures have been used to isolate the nuclear emission. The nuclear near infrared emission can be explained by a combination of dust clouds at different positions and temperatures. The same scans have been used for a tentative
Mediavilla Gradolph, E. et al.
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1986