Hot Very Small dust Grains in NGC 1068 seen in jet induced structures thanks to VLT/NACO adaptive optics

Hot Very Small dust Grains in NGC 1068 seen in jet induced structures thanks to VLT/NACO adaptive optics

We present K, L and M diffraction-limited images of NGC 1068 obtained with NAOS+CONICA at VLT/YEPUN over a 3.5" field around the central engine. Hot dust (Tcol = 550-650 K) is found in three different regions : (a) in the true nucleus, seen as a slightly NS elongated, core of extremely hot dust...

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Hlavní autoři: Rouan, D, Lacombe, F, Gendron, E, Gratadour, D, Clenet, Y, Lagrange, A, Mouillet, D, Boisson, C, Rousset, G, Mugnier, L, Thatte, N, Genzel, R, Gigan, P, Arsenault, R, Kern, P
Médium: Journal article
Jazyk:English
Vydáno: 2003

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