O VI emission in nuclear region of NGC 1068
FUSE Spectra of the nuclear region of NGC 1068 find strong OVI emission consisting of a pair of narrow and broad components. There is a gradient in the velocity field for the narrow O V I component of ∼ 200 kms- 1 from ∼ 2" southwest of the nucleus to
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|Source:||FUTURE DIRECTIONS IN ULTRAVIOLET SPECTROSCOPY: A Conference Inspired by the Accomplishments of the Far Ultraviolet Spectroscopic Explorer Mission|
|01_Zheng_O_VI_emission_in_nuclear_2009.pdf||355.71 kB||Adobe PDF||Request a copy|
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