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Star formation history and dynamical evolution of the solar neighbourhood

Published online by Cambridge University Press:  02 August 2018

Andreas Just  and
Kseniia Sysoliatina
Andreas Just
Affiliation:
Zentrum für Astronomie der Universität Heidelberg, Astronomisches Rechen-Institut, Mönchhofstr. 12-14, 69120 Heidelberg email: just@ari.uni-heidelberg.de
Kseniia Sysoliatina
Affiliation:
Zentrum für Astronomie der Universität Heidelberg, Astronomisches Rechen-Institut, Mönchhofstr. 12-14, 69120 Heidelberg email: just@ari.uni-heidelberg.de
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Abstract

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We used our detailed analytic local disc model to compare predictions in number counts, colour distribuitons and kinematics with a data set extracted from a combination of TGAS and RAVE catalogues. We find generally a very good agreement with some deviations close to the Galactic plane.

Keywords

Galaxy: diskGalaxy: kinematics and dynamicsGalaxy: evolutionGalaxy: solar neighbourhood
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S334: Rediscovering our Galaxy , July 2017 , pp. 310 - 311
Copyright
Copyright © International Astronomical Union 2018 

References

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