Morphology parameters: substructure identification in X-ray galaxy clusters

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dc.contributor.authorParekh, Viral
dc.contributor.authorvan der Heyden, Kurt
dc.contributor.authorFerrari, Chiara
dc.contributor.authorAngus, Garry
dc.contributor.authorHolwerda, Benne
dc.date.accessioned2021-10-08T06:20:34Z
dc.date.available2021-10-08T06:20:34Z
dc.date.issued2015
dc.description.abstractContext. In recent years multi-wavelength observations have shown the presence of substructures related to merging events in a large proportion of galaxy clusters. Clusters can be roughly grouped into two categories – relaxed and non-relaxed – and a proper characterisation of the dynamical state of these systems is crucial for both astrophysical and cosmological studies.
dc.identifier.apacitationParekh, V., van der Heyden, K., Ferrari, C., Angus, G., & Holwerda, B. (2015). Morphology parameters: substructure identification in X-ray galaxy clusters. <i>Astronomy and Astrophysics</i>, 575(4), A127 - 177. http://hdl.handle.net/11427/34306en_ZA
dc.identifier.chicagocitationParekh, Viral, Kurt van der Heyden, Chiara Ferrari, Garry Angus, and Benne Holwerda "Morphology parameters: substructure identification in X-ray galaxy clusters." <i>Astronomy and Astrophysics</i> 575, 4. (2015): A127 - 177. http://hdl.handle.net/11427/34306en_ZA
dc.identifier.citationParekh, V., van der Heyden, K., Ferrari, C., Angus, G. & Holwerda, B. 2015. Morphology parameters: substructure identification in X-ray galaxy clusters. <i>Astronomy and Astrophysics.</i> 575(4):A127 - 177. http://hdl.handle.net/11427/34306en_ZA
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.ris TY - Journal Article AU - Parekh, Viral AU - van der Heyden, Kurt AU - Ferrari, Chiara AU - Angus, Garry AU - Holwerda, Benne AB - Context. In recent years multi-wavelength observations have shown the presence of substructures related to merging events in a large proportion of galaxy clusters. Clusters can be roughly grouped into two categories – relaxed and non-relaxed – and a proper characterisation of the dynamical state of these systems is crucial for both astrophysical and cosmological studies. DA - 2015 DB - OpenUCT DP - University of Cape Town IS - 4 J1 - Astronomy and Astrophysics LK - https://open.uct.ac.za PY - 2015 SM - 0004-6361 SM - 1432-0746 T1 - Morphology parameters: substructure identification in X-ray galaxy clusters TI - Morphology parameters: substructure identification in X-ray galaxy clusters UR - http://hdl.handle.net/11427/34306 ER - en_ZA
dc.identifier.urihttp://hdl.handle.net/11427/34306
dc.identifier.vancouvercitationParekh V, van der Heyden K, Ferrari C, Angus G, Holwerda B. Morphology parameters: substructure identification in X-ray galaxy clusters. Astronomy and Astrophysics. 2015;575(4):A127 - 177. http://hdl.handle.net/11427/34306.en_ZA
dc.language.isoeng
dc.publisher.departmentDepartment of Astronomy
dc.publisher.facultyFaculty of Science
dc.sourceAstronomy and Astrophysics
dc.source.journalissue4
dc.source.journalvolume575
dc.source.paginationA127 - 177
dc.source.urihttps://dx.doi.org/10.1051/0004-6361/201424123
dc.subject.othergalaxies: clusters: intracluster medium
dc.subject.otherX-rays: galaxies: clusters
dc.titleMorphology parameters: substructure identification in X-ray galaxy clusters
dc.typeJournal Article
uct.type.publicationResearch
uct.type.resourceJournal Article
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