Deconstructing Disk Velocity Distribution Functions in the Disk-Mass Survey

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We analyze integral-field ionized gas and stellar line-of-sight kinematics in the context of determining the stellar velocity ellipsoid for spiral galaxies observed by the Disk-Mass Survey. Our new methodology enables us to measure, for the first time, a radial gradient in the ellipsoid ratio sigma_z / sigma_R. Random errors in this decomposition are 15% at two disk scale-lengths.
4 pages, 3 figures, to appear in the proceedings of "Formation and Evolution of Galaxy Disks", Rome, October 2007, Eds. J. Funes and E. M. Corsini

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http://salesiana.dossiersoluciones.com/handle/123456789/147003

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0801.4912
 http://arxiv.org/abs/0801.4912

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arXiv