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Riding the Spiral Waves: Implications of Stellar...
Journal article

Riding the Spiral Waves: Implications of Stellar Migration for the Properties of Galactic Disks

Abstract

Stars in disks of spiral galaxies are usually assumed to remain roughly at their birth radii. This assumption is built into decades of modeling of the evolution of stellar populations in our own Galaxy and in external systems. We present results from self-consistent high-resolution N-body + smooth particle hydrodynamics simulations of disk formation, in which stars migrate across significant galactocentric distances due to resonant scattering with transient spiral arms, while preserving their circular orbits. We investigate the implications of such migrations for observed stellar populations. Radial migration provides an explanation for the observed flatness and spread in the age-metallicity relation and the relative lack of metal-poor stars in the solar neighborhood. The presence of radial migration also prompts rethinking of interpretations of extragalactic stellar population data, especially for determinations of star formation histories.

Authors

Roškar R; Debattista VP; Quinn TR; Stinson GS; Wadsley J

Journal

The Astrophysical Journal, Vol. 684, No. 2, pp. l79–l82

Publisher

American Astronomical Society

Publication Date

September 10, 2008

DOI

10.1086/592231

ISSN

0004-637X

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