The baryonic Tully-Fisher relation and its implication for dark matter halos

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dc.contributor.authorTrachternach, C
dc.contributor.authorde Blok, W J G
dc.contributor.authorMcGaugh, S S
dc.contributor.authorvan der Hulst, J M
dc.contributor.authorDettmar, R-J
dc.date.accessioned2021-10-08T11:01:04Z
dc.date.available2021-10-08T11:01:04Z
dc.date.issued2009
dc.description.abstractThe baryonic Tully-Fisher relation (BTF) is a fundamental relation between baryonic mass and maximum rotation velocity. It can be used to estimate distances, as well as to constrain the properties of dark matter and its relation with the visible matter.
dc.identifier.apacitationTrachternach, C., de Blok, W. J. G., McGaugh, S. S., van der Hulst, J. M., & Dettmar, R. (2009). The baryonic Tully-Fisher relation and its implication for dark matter halos. <i>Astronomy and Astrophysics</i>, 505(2), 577 - 587. http://hdl.handle.net/11427/35079en_ZA
dc.identifier.chicagocitationTrachternach, C, W J G de Blok, S S McGaugh, J M van der Hulst, and R-J Dettmar "The baryonic Tully-Fisher relation and its implication for dark matter halos." <i>Astronomy and Astrophysics</i> 505, 2. (2009): 577 - 587. http://hdl.handle.net/11427/35079en_ZA
dc.identifier.citationTrachternach, C., de Blok, W.J.G., McGaugh, S.S., van der Hulst, J.M. & Dettmar, R. 2009. The baryonic Tully-Fisher relation and its implication for dark matter halos. <i>Astronomy and Astrophysics.</i> 505(2):577 - 587. http://hdl.handle.net/11427/35079en_ZA
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.ris TY - Journal Article AU - Trachternach, C AU - de Blok, W J G AU - McGaugh, S S AU - van der Hulst, J M AU - Dettmar, R-J AB - The baryonic Tully-Fisher relation (BTF) is a fundamental relation between baryonic mass and maximum rotation velocity. It can be used to estimate distances, as well as to constrain the properties of dark matter and its relation with the visible matter. DA - 2009 DB - OpenUCT DP - University of Cape Town IS - 2 J1 - Astronomy and Astrophysics LK - https://open.uct.ac.za PY - 2009 SM - 0004-6361 SM - 1432-0746 T1 - The baryonic Tully-Fisher relation and its implication for dark matter halos TI - The baryonic Tully-Fisher relation and its implication for dark matter halos UR - http://hdl.handle.net/11427/35079 ER - en_ZA
dc.identifier.urihttp://hdl.handle.net/11427/35079
dc.identifier.vancouvercitationTrachternach C, de Blok WJG, McGaugh SS, van der Hulst JM, Dettmar R. The baryonic Tully-Fisher relation and its implication for dark matter halos. Astronomy and Astrophysics. 2009;505(2):577 - 587. http://hdl.handle.net/11427/35079.en_ZA
dc.language.isoeng
dc.publisher.departmentDepartment of Astronomy
dc.publisher.facultyFaculty of Science
dc.sourceAstronomy and Astrophysics
dc.source.journalissue2
dc.source.journalvolume505
dc.source.pagination577 - 587
dc.source.urihttps://dx.doi.org/10.1051/0004-6361/200811136
dc.subject.otherdark matter
dc.subject.othergalaxies: kinematics and dynamics
dc.subject.othergalaxies: dwarf
dc.subject.othergalaxies: fundamental parameters
dc.titleThe baryonic Tully-Fisher relation and its implication for dark matter halos
dc.typeJournal Article
uct.type.publicationResearch
uct.type.resourceJournal Article
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