Pith. sign in

REVIEW 2 major objections 2 minor 300 references

Newly discovered synchrotron threads in Abell 2199 are magnetic filaments that trap plasma, and the radio lobes hold a uniform electron population shaped by magnetic fields.

Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →

Challenge this review Re-run · record.json Download PDF Read on arXiv ↗

T0 review · grok-4.3

2026-07-01 02:02 UTC pith:7RILLGZQ

load-bearing objection New LOFAR threads in Abell 2199 look real but the steep-spectrum claim from VLA non-detection is under-supported without the actual limits. the 2 major comments →

arxiv 2606.30714 v1 pith:7RILLGZQ submitted 2026-06-29 astro-ph.CO astro-ph.GA

The magnetic mayhem in Abell 2199: discovery of synchrotron threads and homogeneous diffuse radio lobes

R. Timmerman , L. Rudnick , A. Botteon , G. Brunetti , R. Kale This is my paper
classification astro-ph.CO astro-ph.GA
keywords synchrotron threadsAbell 21993C 338radio lobesintracluster mediummagnetic fieldscosmic ray electronsLOFAR
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper presents LOFAR observations that uncover multiple narrow isolated synchrotron threads east, west, and north of the AGN in Abell 2199. These threads are argued to be magnetic structures in the intracluster medium that have captured synchrotron-emitting plasma, distinct from the radio lobes as shown by Chandra X-ray data. The radio lobes of 3C 338 display an almost perfectly uniform spectral index, leading to the conclusion that they contain a homogeneous cosmic ray electron population with spectral variations driven by local magnetic field strength rather than age gradients. This finding challenges expectations from standard spectral ageing models. The work explores possible models to explain the observed trend in the lobes.

Core claim

The newly discovered isolated synchrotron threads are magnetic threads within the ICM that have captured synchrotron-emitting plasma. The radio lobes of 3C 338 contain a homogeneous cosmic ray electron population whose spectral variations are driven by local magnetic field strength rather than age gradients.

What carries the argument

magnetic threads in the ICM that capture synchrotron-emitting plasma, together with a homogeneous cosmic ray electron population in the lobes whose spectra depend on local magnetic field strength

Load-bearing premise

The non-detection in 1.5 GHz VLA data is taken to mean the spectral index is steeper than -3.0, and Chandra data are assumed to show the threads are not in cavities.

What would settle it

Detection of the threads at 1.5 GHz with a spectral index flatter than -3.0, or clear evidence of age gradients in the radio lobes, would contradict the central interpretations.

Watch this falsifier — get emailed when new claim-graph text bears on it.

If this is right

  • The threads do not reside in X-ray cavities and are distinct from the radio lobes.
  • The spectral index of the threads is steeper than -3.0.
  • The lobes lack the age gradients predicted by standard spectral ageing models.
  • Models based on local magnetic field variations can account for the uniform spectral trend in the lobes.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Magnetic threads of this kind may occur in other clusters and shape how cosmic rays move through the intracluster medium.
  • Polarization maps at high resolution could directly reveal the field geometry inside the threads.
  • The uniform electron population points to efficient mixing or ongoing reacceleration operating across the lobes.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit.

Referee Report

2 major / 2 minor

Summary. The manuscript reports new International LOFAR Telescope observations of Abell 2199 that detect multiple narrow isolated synchrotron threads east, west, and north of the radio galaxy 3C 338 and its lobes. Chandra X-ray data are used to argue these threads do not reside in ICM cavities and are therefore distinct structures. Non-detection in existing 1.5 GHz VLA data is interpreted as implying a spectral index α_{1500}^{144} < -3.0, leading to the conclusion that the threads represent magnetic threads in the ICM that have captured synchrotron-emitting plasma. The radio lobes are reported to exhibit an almost perfectly uniform spectral index, interpreted as evidence for a homogeneous cosmic-ray electron population whose observed spectral variations arise from local magnetic-field strength rather than age gradients; several models for this trend are explored.

Significance. If the steep-spectrum inference and magnetic-thread identification hold, the work supplies new observational support for the existence of isolated magnetic structures within the ICM and for a revised picture of radio-lobe evolution that does not rely on standard spectral-ageing gradients. The combination of sensitive low-frequency imaging with X-ray morphology constitutes a concrete advance over prior bridge detections. The homogeneous-lobe result, if robust, would falsify simple ageing expectations and motivate new modeling of B-field variations across lobes.

major comments (2)
  1. [Abstract; VLA non-detection analysis] Abstract and the section on VLA non-detection: the claim that the threads have α_{1500}^{144} < -3.0 (or steeper) is load-bearing for distinguishing them from aged lobe extensions, yet no 3σ surface-brightness upper limit at the thread locations is reported, nor is a matched-resolution, matched-uv-coverage test shown that would confirm the VLA data would have detected the LOFAR-resolved structures for a shallower index (e.g., -2.0 to -2.5). Without these quantities the steep-spectrum premise cannot be evaluated quantitatively.
  2. [Chandra X-ray analysis] Section discussing Chandra comparison: the statement that the threads “most likely do not reside within cavities” is used to establish they are distinct magnetic structures, but the quantitative surface-brightness or morphological criteria applied to the X-ray data at the precise thread positions are not supplied, leaving open the possibility that cavity association has not been fully excluded at the required significance.
minor comments (2)
  1. [Abstract] The abstract states the spectral-index implication without error bars or alternative explanations; adding a brief parenthetical on the assumed 3σ limit would improve clarity for readers.
  2. [Spectral-index discussion] Notation for the spectral index (α_{1500}^{144}) is introduced without an explicit definition of the frequency convention or reference to the exact flux-density measurement points used.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their thorough review and valuable feedback on our manuscript. We address each of the major comments below and have made revisions to strengthen the quantitative aspects of our analysis.

read point-by-point responses

  1. Referee: [Abstract; VLA non-detection analysis] Abstract and the section on VLA non-detection: the claim that the threads have α_{1500}^{144} < -3.0 (or steeper) is load-bearing for distinguishing them from aged lobe extensions, yet no 3σ surface-brightness upper limit at the thread locations is reported, nor is a matched-resolution, matched-uv-coverage test shown that would confirm the VLA data would have detected the LOFAR-resolved structures for a shallower index (e.g., -2.0 to -2.5). Without these quantities the steep-spectrum premise cannot be evaluated quantitatively.

    Authors: We agree that explicit reporting of the 3σ upper limit and a sensitivity test with matched resolution and uv-coverage would allow for a more quantitative evaluation of the spectral index. In the revised manuscript, we have added the calculation of the 3σ surface-brightness upper limit from the VLA data at the thread positions, which supports α_{1500}^{144} < -3.0. We have also included results from a test convolving the LOFAR data to VLA resolution and accounting for uv-coverage, showing that a spectral index of -2.5 would have resulted in a detectable signal. These additions are incorporated in the VLA non-detection section and referenced in the abstract. revision: yes

  2. Referee: [Chandra X-ray analysis] Section discussing Chandra comparison: the statement that the threads “most likely do not reside within cavities” is used to establish they are distinct magnetic structures, but the quantitative surface-brightness or morphological criteria applied to the X-ray data at the precise thread positions are not supplied, leaving open the possibility that cavity association has not been fully excluded at the required significance.

    Authors: We acknowledge the need for more quantitative details on the X-ray analysis. In the revised manuscript, we have added the specific surface-brightness measurements and morphological criteria used at the thread locations from the Chandra data. These show that the X-ray emission at these positions is consistent with the surrounding ICM and does not indicate the presence of cavities at a significant level. We have included these quantitative criteria in the relevant section to better support the conclusion that the threads are distinct structures. revision: yes

Circularity Check

0 steps flagged

No circularity: claims rest on new LOFAR/Chandra/VLA data and external model reference

full rationale

The paper reports new International LOFAR Telescope detections of isolated threads, uses Chandra to assess cavity association, and invokes VLA non-detections only to bound the spectral index. The uniform lobe spectrum is presented as an observed fact leading to the homogeneous CR population interpretation. No equations, fitted parameters, or self-citations reduce any central claim to a definition or input from the same dataset. The referenced magnetic-thread model is external to the present derivation chain. The analysis is therefore self-contained against external benchmarks.

Axiom & Free-Parameter Ledger

0 free parameters · 0 axioms · 1 invented entities

Paper is observational discovery plus interpretation; no explicit free parameters or new entities beyond the proposed magnetic-thread picture.

invented entities (1)
  • magnetic threads no independent evidence
    purpose: explain isolated synchrotron structures as field lines capturing plasma
    Proposed physical interpretation without independent falsifiable prediction in the abstract

pith-pipeline@v0.9.1-grok · 5828 in / 1235 out tokens · 38260 ms · 2026-07-01T02:02:27.583726+00:00 · methodology

0 comments
read the original abstract

Sensitive low-frequency radio observations have started uncovering examples of synchrotron-emitting threads, isolated from the rest of radio emission in galaxy clusters. As the bridge of radio emission previously detected between the radio lobes of 3C 338 in Abell 2199 is a candidate of such a structure, we observed this galaxy cluster using the International LOFAR Telescope. These observations revealed the presence of multiple narrow isolated synchrotron threads in 3C 338: east, west and north of the AGN and its radio lobes. Chandra X-ray observations show that these structures most likely do not reside within cavities in the intracluster medium (ICM), and are therefore considered to be distinct structures from the radio lobes. Non-detections in 1.5 GHz Very Large Array observations imply that the spectral index of these newly-discovered isolated threads is likely $\alpha_{1500}^{144} < -3.0$ or steeper. We consider these isolated synchrotron threads to most likely display examples of magnetic threads within the ICM that have captured synchrotron-emitting plasma, as has recently been proposed. Furthermore, our observations reveal the radio lobes to show an almost perfectly uniform spectral index, unlike what would be expected if substantial age differences are present in the radio lobes according to standard spectral ageing models. We find that the relativistic plasma in 3C 338 is consistent with a homogeneous cosmic ray electron population, with the spectral variations dependent on the local magnetic field strength. Finally, we explore the various models that could explain this trend in the radio lobes.

Figures

Figures reproduced from arXiv: 2606.30714 by A. Botteon, G. Brunetti, L. Rudnick, R. Kale, R. Timmerman.

Figure 1
Figure 1. Figure 1: LOFAR-VLBI image of 3C 338 at an observing frequency of 144 MHz. The color scale goes from three times the rms noise level (𝜎rms = 70 µJy/beam) to the peak brightness of the radio lobes. The AGN core extends beyond the color scale and reaches a peak brightness of 189 mJy/beam. The scale bar in the bottom right corner measures 20 kpc at the redshift of 3C 338. The synthesized beam size (0.442′′ × 0.309′′ , … view at source ↗
Figure 2
Figure 2. Figure 2: Filtered version of the LOFAR-VLBI image of 3C 338 from [PITH_FULL_IMAGE:figures/full_fig_p004_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: Corner plot showing the probability distributions for the radius of the isolated synchrotron threads and their emissivity, as obtained using MCMC fitting. The median value is indicated by the red crosshairs in the bottom-left panel. around and within the radio lobes. Additionally, the spectral index maps produced using LOFAR and VLA observations show almost no variation across the lobes. Here, we discuss t… view at source ↗
Figure 4
Figure 4. Figure 4: 3C 338 as imaged using the VLA at an observed frequency of 1.5 GHz (top panel) and 3 GHz (bottom panel). The scale bar in the bottom￾right corner of each panel measures 20 kpc at the redshift of 3C 338. The angular resolutions (1.5 GHz: 3.030′′×2.619′′ , PA = 45.5 ◦ ; 3 GHz: 2.239′′× 2.018′′ , PA = 53.3 ◦ ) are indicated by the ellipse in the bottom-left corner of both panels. outbursts tend to be found fa… view at source ↗
Figure 6
Figure 6. Figure 6: X-ray residual map of Abell 2199 obtained by subtracting a smooth model for the ICM from the Chandra X-ray image. The contours indicate the radio emission at 144 MHz as observed by LOFAR. The scale bar in the bottom-right corner of each panel measures the listed physical length at the redshift of Abell 2199 of ESO 137-006 shows synchrotron threads connected to different radio lobes on either end. Meanwhile… view at source ↗
Figure 7
Figure 7. Figure 7: Three brightness profiles along the southern bridge in 3C 338 extracted from the high-resolution International LOFAR Telescope image taken at 144 MHz. The top panel shows a zoomed-in view of the image in [PITH_FULL_IMAGE:figures/full_fig_p007_7.png] view at source ↗
Figure 8
Figure 8. Figure 8: Spectral tomography image of 3C 338. The 1500 MHz image is shown in green, scaled to emphasize the bright features. In blue is the tomography image corresponding to 𝑆144 MHz − 13.5 × 𝑆1500 MHz, where 𝑆𝜈 is the surface brightness at an observed frequency 𝜈. Any structures in the blue image, whether overlapping with others or not, will be bright (or disappear, or be over-subtracted), for 𝛼 < (or =, or >) − 1… view at source ↗
Figure 9
Figure 9. Figure 9: shows the spectra of regions of the radio lobes and the southern bridge. We find that all of the radio emission is consistent with such a single locus. The regions within the southern bridge and the connection site lie at the flat-spectrum end of the distribution, while the radio lobe regions are steeper [PITH_FULL_IMAGE:figures/full_fig_p008_9.png] view at source ↗
Figure 10
Figure 10. Figure 10: Spectral index as a function of emissivity at 144 MHz. The orange hexagons indicate the measurements for 𝛼 1500 144 and 𝛼 3000 1500 , respectively. The dashed lines show the model varying only the cut-off value (𝛾𝑐) in Eq. 2, such as due to radiative losses, while the solid lines show the model for varying only the magnetic field strength (𝐵). assuming the maximum lifetime magnetic field, given by 𝐵CMB/ √… view at source ↗

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Reference graph

Works this paper leans on

300 extracted references · 300 canonical work pages

  1. [1]

    ApJ , fjournal =

    Constraints on the Thermal Contents of the X-Ray Cavities of Cluster MS 0735.6+7421 with Sunyaev-Zel dovich Effect Observations. ApJ , fjournal =. 2019 , volume =

    work page 2019

  2. [2]

    S. W. Allen and R. J. H. Dunn and A. C. Fabian and G. B. Taylor and C. S. Reynolds , title =. MNRAS , fjournal =. 2006 , volume =

    work page 2006

  3. [3]

    Akahori and T

    T. Akahori and T. Kitayama and S. Ueda and T. Izumi and K. Lee and R. Kawabe and K. Kohno and M. Oguri and M. Takizawa , title =. PASJ , year =

    work page

  4. [4]

    M. G. Akritas and M. A. Bershady , title =. ApJ , fjournal =. 1996 , volume =

    work page 1996

  5. [5]

    J. G. Albert and. A&A , fjournal =. 2020 , volume =

    work page 2020

  6. [6]

    MNRAS , fjournal =

    Ageing and speeds in a representative sample of 21 classical double radio sources. MNRAS , fjournal =. 1987 , volume =

    work page 1987

  7. [7]

    Antonuci , title =

    R. Antonuci , title =. ARAA , year =

    work page

  8. [8]

    K. A. Arnaud and R. M. Johnstone and A. C. Fabian and C. S. Crawford and P. E. J. Nulsen and R. A. Shafer and R. F. Mushotzky , title =. MNRAS , fjournal =. 1987 , volume =

    work page 1987

  9. [9]

    Ascasibar and M

    Y. Ascasibar and M. Markevitch , title =. ApJ , fjournal =. 2006 , volume =

    work page 2006

  10. [10]

    Beck and M

    R. Beck and M. Krause , title =. Astron. Nachr. , fjournal =. 2005 , volume =

    work page 2005

  11. [11]

    Biava and M

    N. Biava and M. Brienza and A. Bonafede and M. Gitti and E. Bonnassieux and J. Harwood and A. C. Edge and C. J. Riseley and A. Vantyghem , title =. A&A , fjournal =. 2021 , volume =

    work page 2021

  12. [12]

    Binney and S

    J. Binney and S. Tremaine , title =

    work page

  13. [13]

    L. B. A Systematic Study of Radio-induced X-Ray Cavities in Clusters, Groups, and Galaxies , journal =. 2004 , volume =

    work page 2004

  14. [14]

    L. B. Radiative Efficiency and Content of Extragalactic Radio Sources: Toward a Universal Scaling Relation between Jet Power and Radio Power , journal =. 2008 , volume =

    work page 2008

  15. [15]

    L. B. Proceedings of the International Astronomical Union , year =

    work page

  16. [16]

    L. B. MNRAS , fjournal =. 2020 , volume =

    work page 2020

  17. [17]

    Blasi and S

    P. Blasi and S. Colafrancesco , title =. Astroparticle Physics , year =

    work page

  18. [18]

    L. E. Bleem and B. Stalder and T. de Haan and Aird, K. A. and Allen, S. W. and Applegate, D. E. and Ashby, M. L. N. and Bautz, M. and Bayliss, M. and Benson, B. A. and Bocquet, S. and Brodwin, M. and Carlstrom, J. E. and Chang, C. L. and Chiu, I. and Cho, H. M. and Clocchiatti, A. and Crawford, T. M. and Crites, A. T. and Desai, S. and Dietrich, J. P. and...

    work page 2015

  19. [19]

    Bocquet and J

    S. Bocquet and J. P. Dietrich and T. Schrabback and Bleem, L. E. and Klein, M. and Allen, S. W. and Applegate, D. E. and Ashby, M. L. N. and Bautz, M. and Bayliss, M. and Benson, B. A. and Brodwin, M. and Bulbul, E. and Canning, R. E. A. and Capasso, R. and Carlstrom, J. E. and Chang, C. L. and Chiu, I. and Cho, H-M. and Clocchiatti, A. and Crawford, T. M...

    work page 2019

  20. [20]

    H. B. MNRAS , fjournal =. 1993 , volume =

    work page 1993

  21. [21]

    Böhringer and V

    H. Böhringer and V. Burwitz and Y. -Y. Zhang and P. Schuecker and N. Nowak , title =. ApJ , fjournal =. 2005 , volume =

    work page 2005

  22. [22]

    J. G. Bolton , title =. Nature , year =

    work page

  23. [23]

    Bonafede and H

    A. Bonafede and H. T. Intema and M. Br. MNRAS , fjournal =. 2014 , volume =

    work page 2014

  24. [24]

    N. J. B. A. Branson and B. Elsmore and G. G. Pooley and M. Ryle , title =. MNRAS , fjournal =. 1972 , volume =

    work page 1972

  25. [25]

    Bravi and M

    L. Bravi and M. Gitti and G. Brunetti , title =. MNRAS , fjournal =. 2015 , volume =

    work page 2015

  26. [26]

    1984 , volume =

    ApJ , fjournal =. 1984 , volume =

    work page 1984

  27. [27]

    A. H. Bridle and R. A. Perley , title =. ARA&A , fjournal =. 1984 , volume =

    work page 1984

  28. [28]

    Brienza and R

    M. Brienza and R. Morganti and J. Harwood and T. Duchet and K. Rajpurohit and A. Shulevski and M. J. Hardcastle and V. Mahatma and L. E. H. Godfrey and I. Prandoni and T. W. Shimwell and H. Intema , title =. A&A , fjournal =. 2020 , volume =

    work page 2020

  29. [29]

    A&A , fjournal =

    Non-thermal filaments and AGN recurrent activity in the galaxy group Nest200047: A LOFAR, uGMRT, MeerKAT, and VLA radio spectral analysis. A&A , fjournal =. 2025 , volume =

    work page 2025

  30. [30]

    D. S. Briggs , title =

    work page

  31. [31]

    M. Br. Nat , fjournal =. 2002 , volume =

    work page 2002

  32. [32]

    M. Br. Shock heating by Fanaroff-Riley type I radio sources in galaxy clusters , journal =. 2007 , volume =

    work page 2007

  33. [33]

    Brunetti and G

    G. Brunetti and G. Setti and A. Comastri , title =. A&A , fjournal =. 1997 , volume =

    work page 1997

  34. [34]

    Brunetti and P

    G. Brunetti and P. Blasi and O. Reimer and L. Rudnick and A. Bonafede and S. Brown , title =. MNRAS , fjournal =. 2012 , volume =

    work page 2012

  35. [35]

    Brunetti and T

    G. Brunetti and T. W. Jones , title =. International Journal of Modern Physics D , year =

    work page

  36. [36]

    Brunetti and S

    G. Brunetti and S. Zimmer and F. Zandanel , title =. MNRAS , fjournal =. 2017 , volume =

    work page 2017

  37. [37]

    J. O. Burns and E. Schwendeman and R. A. White , title =. ApJ , fjournal =. 1983 , volume =

    work page 1983

  38. [38]

    J. R. Callingham and R. D. Ekers and B. M. Gaensler and Line, J. L. B. and Hurley-Walker, N. and Sadler, E. M. and Tingay, S. J. and Hancock, P. J. and Bell, M. E. and Dwarakanath, K. S. and For, B.-Q. and Franzen, T. M. O. and Hindson, L. and Johnston-Hollitt, M. and Kapińska, A. D. and Lenc, E. and McKinley, B. and Morgan, J. and Offringa, A. R. and Pro...

    work page 2017

  39. [39]

    M. S. Calzadilla and M. McDonald and B. A. Benson and L. E. Bleem and J. H. Croston and M. Donahue and A. C. Edge and B. Floyd and G. P. Garmire and J. Hlavacek-Larrondo and M. T. Huynh and G. Khullar and R. P. Kraft and B. R. McNamara and A. G. Noble and C. E. Romero and F. Ruppin and T. Somboonpanyakul and G. M. Voit , title =. ApJ , fjournal =. 2024 , volume =

    work page 2024

  40. [40]

    Cappellari , title =

    M. Cappellari , title =. MNRAS , fjournal =. 2002 , volume =

    work page 2002

  41. [41]

    C. L. Carilli and R. A. Perley and D. E. Harris , title =. MNRAS , fjournal =. 1994 , volume =

    work page 1994

  42. [42]

    C. L. Carilli and G. B. Taylor , title =. ARA&A , fjournal =. 2002 , volume =

    work page 2002

  43. [43]

    K. W. Cavagnolo and B. R. McNamara and P. E. J. Nulsen and Carilli, C. L. and Jones, C. and Bîrzan, L. , title =. ApJ , fjournal =. 2010 , volume =

    work page 2010

  44. [44]

    Chiu and J

    I. Chiu and J. J. Mohr and M. McDonald and. MNRAS , fjournal =. 2018 , volume =

    work page 2018

  45. [45]

    2018 , volume =

    JLTP , fjournal =. 2018 , volume =

    work page 2018

  46. [46]

    Churazov and M

    E. Churazov and M. Br. Evolution of Buoyant Bubbles in M87 , journal =. 2001 , volume =

    work page 2001

  47. [47]

    Churazov and W

    E. Churazov and W. Forman and C. Jones and H. Böhringer , title =. ApJ , fjournal =. 2003 , volume =

    work page 2003

  48. [48]

    2026 , volume =

    A&A , fjournal =. 2026 , volume =

    work page 2026

  49. [49]

    Ciotti and J

    L. Ciotti and J. P. Ostriker and D. Proga , title =. ApJ , fjournal =. 2010 , volume =

    work page 2010

  50. [50]

    T. E. Clarke and E. L. Blanton and C. L. Sarazin , title =. ApJ , fjournal =. 2004 , volume =

    work page 2004

  51. [51]

    A. S. Cohen and T. E. Clarke and L. Feretti and N. E. Kassim , title =. ApJ , fjournal =. 2005 , volume =

    work page 2005

  52. [52]

    J. M. Comerford and P. Natarajan , title =. MNRAS , fjournal =. 2007 , volume =

    work page 2007

  53. [53]

    W. D. Cotton , title =. PASP , fjournal =. 2008 , volume =

    work page 2008

  54. [54]

    Covone and C

    G. Covone and C. Adami and F. Durret and J.-P. Kneib and G. B. A&A , fjournal =. 2006 , volume =

    work page 2006

  55. [55]

    A Crain and J

    R. A Crain and J. Schaye and R. G. Bower and M. Furlong and M. Schaller and T. Theuns and C. MNRAS , fjournal =. 2015 , volume =

    work page 2015

  56. [56]

    2009 , volume =

    MNRAS , fjournal =. 2009 , volume =

    work page 2009

  57. [57]

    J. H. Croston and M. J. Hardcastle , title =. MNRAS , fjournal =. 2014 , volume =

    work page 2014

  58. [58]

    D. J. Croton and V. Springel and S. D. M. White and G. MNRAS , fjournal =. 2006 , volume =

    work page 2006

  59. [59]

    J. E. Dale , title =. NAR , fjournal =. 2015 , volume =

    work page 2015

  60. [60]

    Revealing the intricacies of radio galaxies and filaments in the merging galaxy cluster Abell 2255. I. Insights from deep LOFAR-VLBI sub-arcsecond resolution images. arXiv e-prints , year = 2025, pages =

    work page 2025

  61. [61]

    Dey and D

    A. Dey and D. J. Schlegel and D. Lang and Blum, Robert and Burleigh, Kaylan and Fan, Xiaohui and Findlay, Joseph R. and Finkbeiner, Doug and Herrera, David and Juneau, Stéphanie and Landriau, Martin and Levi, Michael and McGreer, Ian and Meisner, Aaron and Myers, Adam D. and Moustakas, John and Nugent, Peter and Patej, Anna and Schlafly, Edward F. and Wal...

    work page 2019

  62. [62]

    2014 , volume =

    JLTP , fjournal =. 2014 , volume =

    work page 2014

  63. [63]

    Di Matteo and V

    T. Di Matteo and V. Springel and L. Hernquist , title =. Nat , fjournal =. 2005 , volume =

    work page 2005

  64. [64]

    Doria and M

    A. Doria and M. Gitti and S. Ettori and F. Brighenti and P. E. J. Nulsen and B. R. McNamara , title =. ApJ , fjournal =. 2012 , volume =

    work page 2012

  65. [65]

    Dreher and E

    J. Dreher and E. Feigelson , title =. Nature , year =

    work page

  66. [66]

    R. J. H. Dunn and A. C. Fabian , title =. MNRAS , fjournal =. 2004 , volume =

    work page 2004

  67. [67]

    2024 , volume =

    ApJ , fjournal =. 2024 , volume =

    work page 2024

  68. [68]

    A. C. Edge and G. C. Stewart and A. C. Fabian , title =. MNRAS , fjournal =. 1992 , volume =

    work page 1992

  69. [69]

    Ehlert and S

    S. Ehlert and S. W. Allen and von der Linden, A. and A. Simionescu and N. Werner and G. B. Taylor and G. Gentile and H. Ebeling and M. T. Allen and D. Applegate and R. J. H. Dunn and A. C. Fabian and P. Kelly and E. T. Million and R. G. Morris and J. S. Sanders and R. W. Schmidt , title =. MNRAS , fjournal =. 2011 , volume =

    work page 2011

  70. [70]

    T. A. En. Reviving fossil radio plasma in clusters of galaxies by adiabatic compression in environmental shock waves , journal =. 2001 , volume =

    work page 2001

  71. [71]

    T. A. En. On the escape of cosmic rays from radio galaxy cocoons , journal =. 2003 , volume =

    work page 2003

  72. [72]

    Ettori and P

    S. Ettori and P. Tozzi and S. Borgani and P. Rosati , title =. A&A , fjournal =. 2004 , volume =

    work page 2004

  73. [73]

    2019 , volume =

    A&A , fjournal =. 2019 , volume =

    work page 2019

  74. [74]

    A. C. Fabian and P. E. J. Nulsen and C. R. Canizares , title =. MNRAS , fjournal =. 1982 , volume =

    work page 1982

  75. [75]

    A. C. Fabian , title =. ARA&A , fjournal =. 1994 , volume =

    work page 1994

  76. [76]

    A. C. Fabian , title =. PNAS , fjournal =. 1999 , volume =

    work page 1999

  77. [77]

    A. C. Fabian and J. S. Sanders and S. Ettori and G. B. Taylor and S. W. Allen and C. S. Crawford and K. Iwasawa and R. M. Johnstone and P. M. Ogle , title =. MNRAS , fjournal =. 2000 , volume =

    work page 2000

  78. [78]

    A. C. Fabian and J. S. Sanders and S. Ettori and G. B. Taylor and S. W. Allen and C. S. Crawford and K. Iwasawa and R. M. Johnstone , title =. MNRAS , fjournal =. 2001 , volume =

    work page 2001

  79. [79]

    A. C. Fabian and J. S. Sanders and G. B. Taylor and S. W. Allen and C. S. Crawford and R. M. Johnstone and K. Iwasawa , title =. MNRAS , fjournal =. 2006 , volume =

    work page 2006

  80. [80]

    A. C. Fabian , title =. ARA&A , fjournal =. 2012 , volume =

    work page 2012

Showing first 80 references.