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Connecting X-ray absorption and 21 cm neutral hydrogen absorption in obscured radio AGN

Abstract:

Many radio galaxies show the presence of dense and dusty gas near the active nucleus. This can be traced by both 21 cm H I absorption and soft X-ray absorption, offering new insight into the physical nature of the circumnuclear medium of these distant galaxies. To better understand this relationship, we investigate soft X-ray absorption as an indicator for the detection of associated H I absorption, as part of preparation for the First Large Absorption Survey in H I to be undertaken with the ...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

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Publisher copy:
10.1093/mnras/stx1679

Authors


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ORCID:
0000-0002-3005-9738
More by this author
ORCID:
0000-0003-0436-4680
Sadler, EM More by this author
Urquhart, R More by this author
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Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
471
Issue:
3
Pages:
2952-2973
Publication date:
2017-07-06
Acceptance date:
2017-06-30
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Pubs id:
pubs:821061
URN:
uri:1502be6b-bd9c-4011-974b-0f942af2394f
UUID:
uuid:1502be6b-bd9c-4011-974b-0f942af2394f
Local pid:
pubs:821061
Paper number:
3

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