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Warps in Galactic Disks

Published online by Cambridge University Press:  01 June 2007

Gyula I.G. Józsa ,
Franz Kenn ,
Ulrich Klein  and
Thomas A. Oosterloo
Gyula I.G. Józsa
Affiliation:
Argelander Institute for Astronomy (AIfA), Univ. Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany
Franz Kenn
Affiliation:
Argelander Institute for Astronomy (AIfA), Univ. Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany
Ulrich Klein
Affiliation:
Argelander Institute for Astronomy (AIfA), Univ. Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany
Thomas A. Oosterloo
Affiliation:
Netherlands Foundation for Research in Astronomy, Postbus 2, 7990 AA Dwingeloo, The Netherlands Kapteyn Institute, Univ. of Groningen, P.O. Box 800, 9700 AV Groningen, The Netherlands
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Abstract

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We have embarked on a detailed study of the kinematical and morphological structure of HI disks of warped galaxies, which are parametrised by means of kinematic modelling of spectroscopic observations. We present current results and compare them to predictions of theories for warp formation and -maintenance.

Keywords

galaxies: ISMstructurekinematics and dynamicsmethods: data analysis
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S244: Dark Galaxies and Lost Baryons , June 2007 , pp. 360 - 361
Copyright
Copyright © International Astronomical Union 2008

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