Modeling radio circular polarization in the Crab nebula. Issue 1 (14th December 2017)
- Record Type:
- Journal Article
- Title:
- Modeling radio circular polarization in the Crab nebula. Issue 1 (14th December 2017)
- Main Title:
- Modeling radio circular polarization in the Crab nebula
- Authors:
- Bucciantini, N
Olmi, B - Abstract:
- Abstract: In this paper, we present, for the first time, simulated maps of the circularly polarized synchrotron emission from the Crab nebula, using multidimensional state of the art models for the magnetic field geometry. Synchrotron emission is the signature of non-thermal emitting particles, typical of many high-energy astrophysical sources, both Galactic and extragalactic ones. Its spectral and polarization properties allow us to infer key information on the particles distribution function and magnetic field geometry. In recent years, our understanding of pulsar wind nebulae has improved substantially thanks to a combination of observations and numerical models. A robust detection or non-detection of circular polarization will enable us to discriminate between an electron–proton plasma and a pair plasma, clarifying once for all the origin of the radio emitting particles, setting strong constraints on the pair production in pulsar magnetosphere, and the role of turbulence in the nebula. Previous attempts at measuring the circular polarization have only provided upper limits, but the lack of accurate estimates, based on reliable models, makes their interpretation ambiguous. We show here that those results are above the expected values, and that current polarimetric techniques are not robust enough for conclusive result, suggesting that improvements in construction and calibration of next generation radio facilities are necessary to achieve the desired sensitivity.
- Is Part Of:
- Monthly notices of the Royal Astronomical Society. Volume 475:Issue 1(2018)
- Journal:
- Monthly notices of the Royal Astronomical Society
- Issue:
- Volume 475:Issue 1(2018)
- Issue Display:
- Volume 475, Issue 1 (2018)
- Year:
- 2018
- Volume:
- 475
- Issue:
- 1
- Issue Sort Value:
- 2018-0475-0001-0000
- Page Start:
- 822
- Page End:
- 826
- Publication Date:
- 2017-12-14
- Subjects:
- MHD -- polarization -- radiation mechanisms: non-thermal -- relativistic processes -- ISM: individual objects: Crab nebula -- ISM: supernova remnants
Astronomy -- Periodicals
Periodicals
520.5 - Journal URLs:
- http://mnras.oxfordjournals.org/ ↗
http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966 ↗
http://www.blackwell-synergy.com/issuelist.asp?journal=mnr ↗
http://www.blackwell-synergy.com/loi/mnr ↗
http://ukcatalogue.oup.com/ ↗ - DOI:
- 10.1093/mnras/stx3231 ↗
- Languages:
- English
- ISSNs:
- 0035-8711
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 5943.000000
British Library DSC - BLDSS-3PM
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