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Polar Ring Galaxies and the Tully Fisher relation: implications for the dark halo shape

E. Iodice·M. Arnaboldi·F. Bournaud·F. Combes·L. S. Sparke·W. van Driel·M. Capaccioli
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Abstract

We have investigated the Tully-Fisher relation for Polar Ring Galaxies (PRGs), based on near infrared, optical and HI data available for a sample of these peculiar objects. The total K-band luminosity, which mainly comes from the central host galaxy, and the measured HI linewidth at 20% of the peak line flux density, which traces the potential in the polar plane, place most polar rings of the sample far from the Tully-Fisher relation defined for spiral galaxies, with many PRGs showing larger HI linewidths than expected for the observed K band luminosity. This result is confirmed by a larger sample of objects, based on B-band data. This observational evidence may be related to the dark halo shape and orientation in these systems, which we study by numerical modeling of PRG formation and dynamics: the larger rotation velocities observed in PRGs can be explained by a flattened polar halo, aligned with the polar ring.

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E. Iodice, M. Arnaboldi, F. Bournaud, F. Combes, L. S. Sparke, W. van Driel, M. Capaccioli. 2002-11-13. Polar Ring Galaxies and the Tully Fisher relation: implications for the dark halo shape. https://doi.org/10.1086/346107

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