Infrared spectropolarimetry of Seyfert galaxy NGC1068

Infrared spectropolarimetry of Seyfert galaxy NGC1068

Although most of the luminosity of Seyfert galaxy nuclei is emitted in the IR, the relative amounts of thermal dust and non-thermal emission are uncertain. Seyfert galaxies generally have smooth and featureless IR spectra, in contrast to the prominent dust emission features seen in galaxies whose nu...

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Xehetasun bibliografikoak
Egile Nagusiak:	Aitken, D, Bailey, J, Briggs, G, Hough, J, Roche, P
Formatua:	Journal article
Hizkuntza:	English
Argitaratua:	1984

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