Ultraviolet Properties of Low-Redshift AGN Observed with FUSE

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Over the past three years, the Far Ultraviolet Spectroscopic Explorer (FUSE) has obtained 87 spectra of 56 low-redshift (z<0.15) active galactic nuclei (AGN). This sample comprises 53 Type 1 AGN and 3 Type 2. All the Type 1 objects show broad O VI 1034 emission; two of the Type 2s show narrow O VI emission. In addition to O VI, we also identify emission lines due to C III 977, N III 991, S IV 1062,1072,1073, and He II 1085 in many of the Type-1 AGN. Of the Type 1 objects, 30 show intrinsic absorption by the O VI 1032,1038 doublet. Most of these intrinsic absorption systems show multiple components with intrinsic widths of 100 km/s spread over a blue-shifted velocity range of less than 1000 km/s. With the exception of three galaxies (Ton S180, Mrk 478, and Mrk 279), those galaxies in our sample with existing X-ray or longer wavelength UV observations also show C IV absorption and evidence of a soft X-ray warm absorber. In some cases, a UV absorption component has physical properties similar to the X-ray absorbing gas, but in others there is no clear physical correspondence between the UV and X-ray absorbing components. Models in which a thermally driven wind evaporates material from the obscuring torus naturally produce such inhomogeneous flows. Material spanning a broad range of temperatures co-exists in pressure equilibrium. Thus diffuse, highly ionized gas causing X-ray absorption can co-exist with more densely clumped, lower-temperature gas that forms UV absorption lines.
This work is based on data obtained for the Guaranteed Time Team by the NASA-CNES-CSA FUSE mission operated by the Johns Hopkins University. Financial support to U. S. participants has been provided by NASA contract NAS5-32985.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Ultraviolet Properties of Low-Redshift AGN Observed with FUSE does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Ultraviolet Properties of Low-Redshift AGN Observed with FUSE, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet Properties of Low-Redshift AGN Observed with FUSE will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1891588

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.