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Infrared spectroscopy of NGC 1068

  • DePoy D
Springer Berlin Heidelberg, (2008), 106-108
DOI: 10.1007/3-540-19492-4_176
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Abstract

Spectroscopy of the nucleus of the nearby Seyfert 2 galaxy NGC 1068 hasbeen obtained using the IRTF and the facility Cooled-Grating ArraySpectrometer. The data show that the infrared lines are not morebroadened than the optical hydrogen recombination lines, suggesting thatthe presence of an obscured Seyfert 1-like active nucleus is unlikelyunless the visual extinction through any obscuring material present islarger than ≡100 mag.

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APA

DePoy, D. L. (2008). Infrared spectroscopy of NGC 1068. In Active Galactic Nuclei (pp. 106–108). Springer Berlin Heidelberg. https://doi.org/10.1007/3-540-19492-4_176

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