Exploring the GalMer database: bar properties and non-circular motions

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dc.contributor.authorRandriamampandry, T H
dc.contributor.authorDeg, N
dc.contributor.authorCarignan, C
dc.contributor.authorCombes, F
dc.contributor.authorSpekkens, K
dc.date.accessioned2021-10-08T06:20:06Z
dc.date.available2021-10-08T06:20:06Z
dc.date.issued2016
dc.description.abstractContext. We use Tree-SPH simulations from the GalMer database to characterize and quantify the non-circular motions induced by the presence of bar-like structures on the observed rotation curve of barred galaxies derived from empirical models of their line-of-sight velocity maps. The GalMer database consists of SPH simulations of galaxies spanning a wide range of morphological types and sizes.
dc.identifier.apacitationRandriamampandry, T. H., Deg, N., Carignan, C., Combes, F., & Spekkens, K. (2016). Exploring the GalMer database: bar properties and non-circular motions. <i>Astronomy and Astrophysics</i>, 594(4), A86 - 177. http://hdl.handle.net/11427/34204en_ZA
dc.identifier.chicagocitationRandriamampandry, T H, N Deg, C Carignan, F Combes, and K Spekkens "Exploring the GalMer database: bar properties and non-circular motions." <i>Astronomy and Astrophysics</i> 594, 4. (2016): A86 - 177. http://hdl.handle.net/11427/34204en_ZA
dc.identifier.citationRandriamampandry, T.H., Deg, N., Carignan, C., Combes, F. & Spekkens, K. 2016. Exploring the GalMer database: bar properties and non-circular motions. <i>Astronomy and Astrophysics.</i> 594(4):A86 - 177. http://hdl.handle.net/11427/34204en_ZA
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.ris TY - Journal Article AU - Randriamampandry, T H AU - Deg, N AU - Carignan, C AU - Combes, F AU - Spekkens, K AB - Context. We use Tree-SPH simulations from the GalMer database to characterize and quantify the non-circular motions induced by the presence of bar-like structures on the observed rotation curve of barred galaxies derived from empirical models of their line-of-sight velocity maps. The GalMer database consists of SPH simulations of galaxies spanning a wide range of morphological types and sizes. DA - 2016 DB - OpenUCT DP - University of Cape Town IS - 4 J1 - Astronomy and Astrophysics LK - https://open.uct.ac.za PY - 2016 SM - 0004-6361 SM - 1432-0746 T1 - Exploring the GalMer database: bar properties and non-circular motions TI - Exploring the GalMer database: bar properties and non-circular motions UR - http://hdl.handle.net/11427/34204 ER - en_ZA
dc.identifier.urihttp://hdl.handle.net/11427/34204
dc.identifier.vancouvercitationRandriamampandry TH, Deg N, Carignan C, Combes F, Spekkens K. Exploring the GalMer database: bar properties and non-circular motions. Astronomy and Astrophysics. 2016;594(4):A86 - 177. http://hdl.handle.net/11427/34204.en_ZA
dc.language.isoeng
dc.publisher.departmentDepartment of Astronomy
dc.publisher.facultyFaculty of Science
dc.sourceAstronomy and Astrophysics
dc.source.journalissue4
dc.source.journalvolume594
dc.source.paginationA86 - 177
dc.source.urihttps://dx.doi.org/10.1051/0004-6361/201629081
dc.subject.otherdark matter
dc.subject.othergalaxies: kinematics and dynamics
dc.subject.othergalaxies: structure
dc.subject.othergalaxies: spiral
dc.titleExploring the GalMer database: bar properties and non-circular motions
dc.typeJournal Article
uct.type.publicationResearch
uct.type.resourceJournal Article
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