SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:su-124793"
 

Search: onr:"swepub:oai:DiVA.org:su-124793" > Linear polarization...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Linear polarization structures in LOFAR observations of the interstellar medium in the 3C 196 field

Jelić, V. (author)
de Bruyn, A. G. (author)
Pandey, V. N. (author)
show more...
Mevius, M. (author)
Haverkorn, M. (author)
Brentjens, M. A. (author)
Koopmans, L. V. E. (author)
Zaroubi, S. (author)
Abdalla, F. B. (author)
Asad, K. M. B. (author)
Bus, S. (author)
Chapman, E. (author)
Ciardi, B. (author)
Fernandez, E. R. (author)
Ghosh, A. (author)
Harker, G. (author)
Iliev, I. T. (author)
Jensen, Hannes (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Kazemi, S. (author)
Mellema, Garrelt (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Offringa, A. R. (author)
Patil, A. H. (author)
Vedantham, H. K. (author)
Yatawatta, S. (author)
show less...
 (creator_code:org_t)
2015-11-05
2015
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 583
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Aims: This study aims to characterize linear polarization structures in LOFAR observations of the interstellar medium (ISM) in the 3C 196 field, one of the primary fields of the LOFAR-Epoch of Reionization key science project.Methods: We have used the high band antennas (HBA) of LOFAR to image this region and rotation measure (RM) synthesis to unravel the distribution of polarized structures in Faraday depth.Results: The brightness temperature of the detected Galactic emission is 5-15 K in polarized intensity and covers the range from -3 to +8 rad m(-2) in Faraday depth. The most interesting morphological feature is a strikingly straight filament at a Faraday depth of +0.5 rad m(-2) running from north to south, right through the centre of the field and parallel to the Galactic plane. There is also an interesting system of linear depolarization canals conspicuous in an image showing the peaks of Faraday spectra. We used the Westerbork Synthesis Radio Telescope (WSRT) at 350 MHz to image the same region. For the first time, we see some common morphology in the RM cubes made at 150 and 350 MHz. There is no indication of diffuse emission in total intensity in the interferometric data, in line with results at higher frequencies and previous LOFAR observations. Based on our results, we determined physical parameters of the ISM and proposed a simple model that may explain the observed distribution of the intervening magneto-ionic medium.Conclusions: The mean line-of-sight magnetic field component, B-parallel to, is determined to be 0.3 +/- 0.1 mu G and its spatial variation across the 3C 196 field is 0.1 mu G. The filamentary structure is probably an ionized filament in the ISM, located somewhere within the Local Bubble. This filamentary structure shows an excess in thermal electron density (n(e)B(parallel to) > 6.2 cm(-3) mu G) compared to its surroundings.

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Keyword

ISM: general
ISM: magnetic fields
ISM: structure
radio continuum: ISM
techniques: interferometric
techniques: polarimetric

Publication and Content Type

ref (subject category)
art (subject category)

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view