# Kinematics of massive star ejecta in the Milky Way as traced by 26Al

@article{Kretschmer2013KinematicsOM,
title={Kinematics of massive star ejecta in the Milky Way as traced by 26Al},
author={Karsten Kretschmer and Roland Diehl and Martin G H Krause and Andreas Burkert and Katharina M. Fierlinger and Ortwin Gerhard and J. Greiner and Wei Wang},
journal={Astronomy and Astrophysics},
year={2013},
volume={559},
pages={1-11}
}
Context. Massive stars form in groups and their winds and supernova explosions create superbubbles up to kpc in size. The fate of their ejecta is of vital importance for the dynamics of the interstellar medium, for chemical evolution models, and the chemical enrichment of galactic halos and the intergalactic medium. However, ejecta kinematics and the characteristic scales in space and time have not been explored in great detail beyond 10 ka. Aims. Through measurement of radioactive 26 Al with… Expand

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