- 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 ...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
-
(pdf, 6.1mb)
-
- Publisher copy:
- 10.1093/mnras/stx1679
-
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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
- Copyright holder:
- Moss et al.
- Copyright date:
- 2017
- Notes:
- © 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.
Journal article
Connecting X-ray absorption and 21 cm neutral hydrogen absorption in obscured radio AGN
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