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Exploring the properties of low-frequency radio emission and magnetic fields in a sample of compact galaxy groups using the LOFAR Two-Metre Sky Survey (LoTSS)

Nikiel-Wroczynski, N. (author)
Jagiellonian University in Kraków, Poland
Berger, A. (author)
Ruhr-Universität Bochum
Herrera Ruiz, N. (author)
Ruhr-Universität Bochum
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Bomans, D. (author)
Ruhr-Universität Bochum
Blex, S. (author)
Ruhr-Universität Bochum
Horellou, Cathy, 1967 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Paladino, R. (author)
Istituto nazionale di astrofisica (INAF)
Becker, A. (author)
Ruhr-Universität Bochum
Miskolczi, A. (author)
Ruhr-Universität Bochum
Beck, R. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Chy, K. T. (author)
Jagiellonian University in Kraków, Poland
Dettmar, R. -J. (author)
Ruhr-Universität Bochum
Heald, G. (author)
Commonwealth Scientific and Industrial Research Organisation (CSIRO)
Heesen, V. (author)
Universität Hamburg,University of Hamburg
Jamrozy, M. (author)
Jagiellonian University in Kraków, Poland
Shimwell, T. W. (author)
Netherlands Institute for Radio Astronomy (ASTRON)
Tasse, C. (author)
Paris Diderot University, France
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 (creator_code:org_t)
2019-02-19
2019
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 622
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We use the LOFAR Two-metre Sky Survey (LoTSS) Data Release I to identify the groups of galaxies (and individual galaxies) from the Hickson compact groups (HCG) and magnitude-limited compact groups (MLCG) samples that emit at the frequency of 150 MHz, characterise their radio emission (extended or limited to the galaxies), and compare new results to earlier observations and theoretical predictions. The detection of 73 systems (and 7 more - probably) out of 120, of which as many as 17 show the presence of extended radio structures, confirms the previous hypothesis of the common character of the magnetic field inside galaxy groups and its detectability. In order to investigate the future potential of low-frequency radio studies of galaxy groups, we also present a more detailed insight into four radio-emitting systems, for which the strength of the magnetic field inside their intergalactic medium (IGM) is calculated. The estimated values are comparable to that found inside star-forming galaxies, suggesting a dynamical and evolutionary importance of the magnetic field in galaxy groups.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Annan fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Other Physics Topics (hsv//eng)
MEDICIN OCH HÄLSOVETENSKAP  -- Medicinsk bioteknologi -- Biomedicinsk laboratorievetenskap/teknologi (hsv//swe)
MEDICAL AND HEALTH SCIENCES  -- Medical Biotechnology -- Biomedical Laboratory Science/Technology (hsv//eng)

Keyword

Galaxies: groups: general
Galaxies: magnetic fields
Radio continuum: galaxies
Magnetic fields

Publication and Content Type

art (subject category)
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