Resolving the coronal line region of NGC 1068 with near-infrared integral field spectroscopy
We present adaptive optics-assisted J- and K-band integral field spectroscopy of the inner 300 × 300 pc of the Seyfert 2 galaxy NGC 1068. The data were obtained with the Gemini Near-infrared Integral-Field Spectrograph integral field unit spectrometer, w
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Mazzalay_Resolving_the_coronal_line_2013.pdf||4.66 MB||Adobe PDF||Request a copy|
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