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

Journal Article

2009

Permanent link to this Item
http://hdl.handle.net/11427/35079
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TrachternachC_baryonic_Tully_2009.pdf (1.33 MB)
Authors
Trachternach, C
de Blok, W J G
McGaugh, S S
van der Hulst, J M
Dettmar, R-J
Journal Title

Astronomy and Astrophysics

Link to Journal
https://dx.doi.org/10.1051/0004-6361/200811136
Journal ISSN
Volume Title
Publisher
Publisher
Department
Department of Astronomy
Faculty
Faculty of Science
License
Series
Abstract
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.
Description
Keywords
dark matter
galaxies: kinematics and dynamics
galaxies: dwarf
galaxies: fundamental parameters

Reference:

Trachternach, 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. Astronomy and Astrophysics. 505(2):577 - 587. http://hdl.handle.net/11427/35079

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