Measuring the intracluster medium velocity structure within the A3266 galaxy cluster Article Swipe
E. Gatuzz
,
J. Sanders
,
A. Liu
,
A. Fabian
,
C. Pinto
,
H. R. Russell
,
D. Eckert
,
Stephen Walker
,
J. ZuHone
,
Rabindra N. Mohapatra
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/202451640
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/202451640
We present a detailed analysis of the velocity structure of the hot intracluster medium (ICM) within the A3266 galaxy cluster, including new observations taken between June and November 2023. Firstly, morphological structures within the galaxy cluster were examined using a Gaussian gradient magnitude (GGM) and an adaptively smoothed GGM filter applied to the EPIC-pn X-ray image. Then, we applied a novel XMM-Newton EPIC-pn energy scale calibration, which uses instrumental Cu K α as a reference for the line emission, to measure the line-of-sight velocities of hot gas within the system. This approach enabled us to create two-dimensional projected maps for velocity, temperature, and metallicity, showing that the hot gas displays a redshifted systemic velocity relative to the cluster redshift across all fields of view. Further analysis of the velocity distribution through non-overlapping circular regions demonstrates consistent redshifted velocities extending up to 1125 kpc from the cluster core. Additionally, the velocity distribution was assessed along regions following surface brightness discontinuities, where we observed redshifted velocities in all regions, with the largest velocities reaching 768 ± 284 km/s. Moreover, we computed the velocity probability density function (PDF) from the velocity map. We applied a normality test, finding that the PDF adheres to an unimodal normal distribution consistent with theoretical predictions. Lastly, we computed a velocity structure function for this system using the measured line-of-sight velocities. These insights advance our understanding of the dynamic processes within the A3266 galaxy cluster and contribute to our broader knowledge of ICM behavior in merging galaxy clusters.
Related Topics
Concepts
Physics
Intracluster medium
Astrophysics
Galaxy cluster
Cluster (spacecraft)
Brightest cluster galaxy
Astronomy
Type-cD galaxy
Galaxy
Velocity dispersion
Programming language
Computer science
Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1051/0004-6361/202451640
- OA Status
- hybrid
- Cited By
- 4
- References
- 48
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4404479897
All OpenAlex metadata
Raw OpenAlex JSON
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https://openalex.org/W4404479897Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1051/0004-6361/202451640Digital Object Identifier
- Title
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Measuring the intracluster medium velocity structure within the A3266 galaxy clusterWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
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2024Year of publication
- Publication date
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2024-11-18Full publication date if available
- Authors
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E. Gatuzz, J. Sanders, A. Liu, A. Fabian, C. Pinto, H. R. Russell, D. Eckert, Stephen Walker, J. ZuHone, Rabindra N. MohapatraList of authors in order
- Landing page
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https://doi.org/10.1051/0004-6361/202451640Publisher landing page
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YesWhether a free full text is available
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hybridOpen access status per OpenAlex
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https://doi.org/10.1051/0004-6361/202451640Direct OA link when available
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Physics, Intracluster medium, Astrophysics, Galaxy cluster, Cluster (spacecraft), Brightest cluster galaxy, Astronomy, Type-cD galaxy, Galaxy, Velocity dispersion, Programming language, Computer scienceTop concepts (fields/topics) attached by OpenAlex
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4Total citation count in OpenAlex
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2025: 4Per-year citation counts (last 5 years)
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10Other works algorithmically related by OpenAlex
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