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

Astronomy and Astrophysics

Volumn 417, Issue 1, 2004, Pages

  Rouan, D ^a   Lacombe, F ^a   Gendron, E ^a   Gratadour, D ^a,c   Clenet Y ^a   Lagrange, A M ^b   Mouillet, D ^b   Boisson, C ^e   Rousset, G ^c   Fusco, T ^c   Mugnier, L ^c   Sechaud M ^c   Thatte, N ^d   Genzel, R ^a   Gigan, P ^a   Arsenault, R ^a,f   Kern, P ^b  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b LABORATOIRE D ASTROPHYSIQUE   (France)

^c ONERA   (France)

^d MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^e UNIVERSITÉ PARIS DIDEROT   (France)

^f EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Galaxies: active; Galaxies: dust; Galaxies: NGC 1068; Galaxies: nuclei; Galaxies: Seyfert; Infrared: galaxies; Instrumentation: adaptive optics; Instrumentation: near and mid IR

Indexed keywords

ADAPTIVE OPTICS; DIAMONDS; DIFFRACTION; DUST; GALAXIES; IMAGE ANALYSIS; INFRARED RADIATION; INTEGRATION; MORPHOLOGY; POLARIZATION; PROBABILITY; SPECTRUM ANALYSIS;

GALAXIES: ACTIVE; GALAXIES: DUST; GALAXIES: NGC 1068; GALAXIES: NUCLEI; GALAXIES: SEYFERT; INFRARED: GALAXIES; INSTRUMENTATION: ADAPTIVE OPTICS; INSTRUMENTATION: NEAR- AND MID-IR;

ASTRONOMY;

EID: 12144289436     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040029     Document Type: Article

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