Journal article
WISDOM project – IV. A molecular gas dynamical measurement of the supermassive black hole mass in NGC 524
- Abstract:
-
We present high angular resolution (0.3 arcsec or 37 pc) Atacama Large Millimeter/submillimeter Array observations of the CO(2–1) line emission from a central disc in the early-type galaxy NGC 524. This disc is shown to be dynamically relaxed, exhibiting ordered rotation about a compact 1.3 mm continuum source, which we identify as emission from an active supermassive black hole (SMBH). There is a hole at the centre of the disc slightly larger than the SMBH sphere of influence. An azimuthal d...
Expand abstract
- Publication status:
- Published
- Peer review status:
- Peer reviewed
Actions
Access Document
- Files:
-
-
(Version of record, pdf, 13.0MB)
-
- Publisher copy:
- 10.1093/mnras/stz625
Why is the content I wish to access not available via ORA?
Bibliographic data (the information relating to research outputs) and full-text items (e.g. articles, theses, reports, etc.) arrive in ORA from several different sources. Unfortunately we are not able to make available the full-text for every research output.
Please contact the ORA team (
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
Content may be unavailable for the following four reasons
-
Version unsuitable
-
We have not obtained a suitable full-text for a given research output. See this page for more information.
-
Recently completed
-
Sometimes content is held in ORA but is unavailable for a fixed period of time to comply with the policies and wishes of rights holders.
-
Permissions
-
All content made available in ORA should comply with relevant rights, such as copyright. See this page for more information.
-
Clearance
-
Some thesis volumes scanned as part of the digitisation scheme funded by Dr Leonard Polonsky are currently unavailable due to sensitive material or uncleared third-party copyright content. We are attempting to contact authors whose theses are affected.
Alternative access to the full-text
You may be able to access the full-text directly from the publisher's website using the 'Publisher Copy' link in the 'Links & Downloads' box from a research output's ORA record page. This method may require an institutional or individual subscription to the journal/resource.
Authors
Bibliographic Details
- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 485
- Issue:
- 3
- Pages:
- 4359–4374
- Publication date:
- 2019-03-07
- Acceptance date:
- 2019-02-26
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- Source identifiers:
-
983950
Item Description
- Keywords:
- Pubs id:
-
pubs:983950
- UUID:
-
uuid:3b35b649-9340-4152-bed5-b72f710357fe
- Local pid:
- pubs:983950
- Deposit date:
- 2019-03-22
Terms of use
- Copyright holder:
- Smith et al
- Copyright date:
- 2019
- Notes:
- Copyright © 2019 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.
If you are the owner of this record, you can report an update to it here: Report update to this record