The Galactic Scale UV Outflow Discovered In High S/N HST COS Observations Of IRAS F04250-5718

Details The Galactic Scale UV Outflow Discovered In High S/N HST COS Observations Of IRAS F04250-5718 The Galactic Scale UV Outflow Discovered In High S/N HST COS Observations Of IRAS F04250-5718

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21743203e&link_type=abstract

American Astronomical Society, AAS Meeting #217, #432.03; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

We report on the discovery of a large scale AGN outflow in IRAS F04250-5718. Analysis of absorption troughs in high S/N data from HST COS observations made in June of 2010 reveals an outflow 50 kpc from the central source. The outflow is unusual in both its extremely large distance and its photoionization structure. While multiple ionization components are necessary to fit data in X-ray absorption studies, a single ionization parameter normally suffices for UV studies. In this outflow, however, we require at least two ionization parameters to fit the UV data.

Affiliated with

Also associated with

No associations

Rating

The Galactic Scale UV Outflow Discovered In High S/N HST COS Observations Of IRAS F04250-5718 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 The Galactic Scale UV Outflow Discovered In High S/N HST COS Observations Of IRAS F04250-5718, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Galactic Scale UV Outflow Discovered In High S/N HST COS Observations Of IRAS F04250-5718 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1404398