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Star formation and jet-induced coronal lines near the core of NGC 1068
2011
Astronomy and Astrophysics
Context. Active galactic nuclei (AGNs) are very luminous galaxies from the ultraviolet (UV) to the far infrared (FIR). To study regions near the core, which are dominated by dust, IR is the perfect spectral range because of the lower optical depth of the dust. However, these galaxies are usually distant, and the structures near the core are faint compared to the central source. High resolution and high contrast are mandatory to study the inner structures of AGNs and better understand the
doi:10.1051/0004-6361/201116943
fatcat:5ufbnth5frfntb7gqzrmwe75sa