- Abstract:
-
Observations of binary stars containing an accreting black hole or neutron star often show x-ray emission extending to high energies (>10 kilo--electron volts), which is ascribed to an accretion disk corona of energetic particles akin to those seen in the solar corona. Despite their ubiquity, the physical conditions in accretion disk coronae remain poorly constrained. Using simultaneous infrared, optical, x-ray, and radio observations of the Galactic black hole system V404 Cygni, showing a...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Publisher copy:
- 10.1126/science.aan0249
-
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.
- Publisher:
- American Association for the Advancement of Science Publisher's website
- Journal:
- Science Journal website
- Volume:
- 358
- Issue:
- 6368
- Publication date:
- 2017-12-08
- Acceptance date:
- 2017-11-03
- DOI:
- ISSN:
-
0036-8075 and 1095-9203
- Pubs id:
-
pubs:810943
- URN:
-
uri:ac9fbe37-e275-4577-b837-7914aedbd690
- UUID:
-
uuid:ac9fbe37-e275-4577-b837-7914aedbd690
- Local pid:
- pubs:810943
- Language:
- English
- Keywords:
- Copyright holder:
- Dallilar et al.
- Copyright date:
- 2017
- Notes:
- © The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. An erratum for this article is available at: 10.1126/science.aat9270
Journal article
A precise measurement of the magnetic field in the corona of the black hole binary V404 Cygni
Actions
Access Document
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
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
Item Description
Terms of use
If you are the owner of this record, you can report an update to it here: Report update to this record