Far Ultraviolet Outflow Properties of IZw1

Details Far Ultraviolet Outflow Properties of IZw1 Far Ultraviolet Outflow Properties of IZw1

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.4413r&link_type=abstract

American Astronomical Society, AAS Meeting #211, #44.13; Bulletin of the American Astronomical Society, Vol. 39, p.794

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a detailed look into the basic properties of the O VI absorption in the outflow gas from the Seyfert 1 galaxy I Zw 1 using data from the Far Ultraviolet Spectroscopic Explorer. This outflow shows a two-component ionization structure in the X rays, and previous work shows the UV absorption likely associated with the low-ionization component. We use continuum and emission line fits to measure the absorption properties from the normalized spectrum. We compare these properties to those already measured in C IV absorption data from the Faint Object Spectrograph on the Hubble Space Telescope.

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