Near infrared surface photometry of NGC 1068.

Mediavilla Gradolph, E.; Sanchez Magro, C.
Referencia bibliográfica

Structure and evolution of active galactic nuclei, p. 633 - 636

Fecha de publicación:
0
1986
Número de autores
2
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
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 detection of the ring in the L band.