Radio Galaxy Zoo: observational evidence for environment as the cause of radio source asymmetry

P. E. Rodman, R. J. Turner, S. S. Shabala, J. K. Banfield, O. I. Wong, H. Andernach, A. F. Garon, A. D. Kapinska, R. P. Norris, L. Rudnick

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

We investigate the role of environment on radio galaxy properties by constructing a sample of large (greater than or similar to 100 kpc), nearby (z <0.3) radio sources identified as part of the Radio Galaxy Zoo citizen science project. Our sample consists of 16 Fanaroff-Riley Type II (FR-II) sources, 6 FR-I sources, and 1 source with a hybrid morphology. FR-I sources appear to be hosted by more massive galaxies, consistent with previous studies. In the FR-II sample, we compare the degree of asymmetry in radio lobe properties to asymmetry in the radio source environment, quantified through optical galaxy clustering. We find that the length of radio lobes in FR-II sources is anticorrelated with both galaxy clustering and lobe luminosity. These results are in quantitative agreement with predictions from radio source dynamical models and suggest that galaxy clustering provides a useful proxy for the ambient gas density distribution encountered by the radio lobes.

Original languageEnglish
Pages (from-to)5625-5641
Number of pages17
JournalMonthly Notices of the Royal Astronomical Society
Volume482
Issue number4
DOIs
Publication statusPublished - Feb 2019

Cite this

Rodman, P. E. ; Turner, R. J. ; Shabala, S. S. ; Banfield, J. K. ; Wong, O. I. ; Andernach, H. ; Garon, A. F. ; Kapinska, A. D. ; Norris, R. P. ; Rudnick, L. / Radio Galaxy Zoo : observational evidence for environment as the cause of radio source asymmetry. In: Monthly Notices of the Royal Astronomical Society. 2019 ; Vol. 482, No. 4. pp. 5625-5641.
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Rodman, PE, Turner, RJ, Shabala, SS, Banfield, JK, Wong, OI, Andernach, H, Garon, AF, Kapinska, AD, Norris, RP & Rudnick, L 2019, 'Radio Galaxy Zoo: observational evidence for environment as the cause of radio source asymmetry' Monthly Notices of the Royal Astronomical Society, vol. 482, no. 4, pp. 5625-5641. https://doi.org/10.1093/mnras/sty3070

Radio Galaxy Zoo : observational evidence for environment as the cause of radio source asymmetry. / Rodman, P. E.; Turner, R. J.; Shabala, S. S.; Banfield, J. K.; Wong, O. I.; Andernach, H.; Garon, A. F.; Kapinska, A. D.; Norris, R. P.; Rudnick, L.

In: Monthly Notices of the Royal Astronomical Society, Vol. 482, No. 4, 02.2019, p. 5625-5641.

Research output: Contribution to journalArticle

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AU - Rodman, P. E.

AU - Turner, R. J.

AU - Shabala, S. S.

AU - Banfield, J. K.

AU - Wong, O. I.

AU - Andernach, H.

AU - Garon, A. F.

AU - Kapinska, A. D.

AU - Norris, R. P.

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AB - We investigate the role of environment on radio galaxy properties by constructing a sample of large (greater than or similar to 100 kpc), nearby (z <0.3) radio sources identified as part of the Radio Galaxy Zoo citizen science project. Our sample consists of 16 Fanaroff-Riley Type II (FR-II) sources, 6 FR-I sources, and 1 source with a hybrid morphology. FR-I sources appear to be hosted by more massive galaxies, consistent with previous studies. In the FR-II sample, we compare the degree of asymmetry in radio lobe properties to asymmetry in the radio source environment, quantified through optical galaxy clustering. We find that the length of radio lobes in FR-II sources is anticorrelated with both galaxy clustering and lobe luminosity. These results are in quantitative agreement with predictions from radio source dynamical models and suggest that galaxy clustering provides a useful proxy for the ambient gas density distribution encountered by the radio lobes.

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KW - GAS

KW - MORPHOLOGY

KW - FEEDBACK

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JF - Monthly Notices of the Royal Astronomical Society

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