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Figure 1. Full FUV spectrum of IRAS F22456−5125 obtained by COS. The major absorption troughs related to the intrinsic absorber are labeled. The green line represents our fit to the non-absorbed emission model (see Section 2.3).
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Journal Article
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DOI
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A 10 kpc SCALE SEYFERT GALAXY OUTFLOW: HST/COS OBSERVATIONS OF IRAS F22456–5125
[...]
B. Borguet
1
,
Douglas Edmonds
1
,
Nahum Arav
1
,
Jay P. Dunn
2
,
Gerard A. Kriss
3
,
Gerard A. Kriss
4
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+2 more
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Institutions (4)
Virginia Tech
1
,
Georgia Perimeter College
2
,
Johns Hopkins University
3
,
Space Telescope Science Institute
4
01 Jun 2012
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The Astrophysical Journal