The Distribution of Young Stars and Metals in Simulated Cosmological Disk Galaxies

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics

Scientific paper

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To appear in "From the First Structures to the Universe Today"; Proceedings of 2nd Workshop on Numerical and Observational Ast

Scientific paper

We examine the distribution of young stars associated with the spiral arms of a simulated L* cosmological disk galaxy. We find age patterns orthogonal to the arms which are not inconsistent with the predictions of classical density wave theory, a view further supported by recent observations of face-on Grand Design spirals such as M51. The distribution of metals within a simulated ~0.1L* disk is presented, reinforcing the link between star formation, the age-metallicity relation, and the metallicity distribution function.

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