Journal article
A precise measurement of the magnetic field in the corona of the black hole binary V404 Cygni
- 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...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Publisher copy:
- 10.1126/science.aan0249
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Authors
Bibliographic Details
- 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:
-
1095-9203 and 0036-8075
- Pmid:
-
29217570
- Source identifiers:
-
810943
Item Description
- Language:
- English
- Keywords:
- Pubs id:
-
pubs:810943
- UUID:
-
uuid:ac9fbe37-e275-4577-b837-7914aedbd690
- Local pid:
- pubs:810943
- Deposit date:
- 2019-01-02
Terms of use
- 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
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