Star formation history and dynamical evolution of the solar neighbourhood
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.
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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) Konferenzschrift |
| Sprache: | Englisch |
| Veröffentlicht: |
02 August 2018
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| In: |
Proceedings of the International Astronomical Union
Year: 2017, Jahrgang: 13, Heft: S334, Pages: 310-311 |
| ISSN: | 1743-9221 |
| DOI: | 10.1017/S1743921317008158 |
| Online-Zugang: | Verlag, Volltext: https://doi.org/10.1017/S1743921317008158 Verlag, Volltext: https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/star-formation-history-and-dynamical-evolution-of-the-solar-neighbourhood/009B401B5E980AFCBE1BB996D6FC762F 
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| Verfasserangaben: | Andreas Just and Kseniia Sysoliatina |
| Zusammenfassung: | 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. |
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| Beschreibung: | Gesehen am 03.09.2019 |
| Beschreibung: | Online Resource |
| ISSN: | 1743-9221 |
| DOI: | 10.1017/S1743921317008158 |