Hostname: page-component-78c5997874-fbnjt Total loading time: 0 Render date: 2024-11-19T12:33:59.616Z Has data issue: false hasContentIssue false
  • English
  • Français

The evolution history of the extended solar neighbourhood

Published online by Cambridge University Press:  07 March 2018

Andreas Just ,
Kseniia Sysoliatina  and
Ioanna Koutsouridou
Andreas Just
Affiliation:
Zentrum für Astronomie der Universität Heidelberg, Astronomisches Rechen-Institut, Mönchhofstr. 12-14, 69120 Heidelberg email: [email protected]
Kseniia Sysoliatina
Affiliation:
Zentrum für Astronomie der Universität Heidelberg, Astronomisches Rechen-Institut, Mönchhofstr. 12-14, 69120 Heidelberg email: [email protected]
Ioanna Koutsouridou
Affiliation:
Zentrum für Astronomie der Universität Heidelberg, Astronomisches Rechen-Institut, Mönchhofstr. 12-14, 69120 Heidelberg email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Our detailed analytic local disc model (JJ-model) quantifies the interrelation between kinematic properties (e.g. velocity dispersions and asymmetric drift), spatial parameters (scale-lengths and vertical density profiles), and properties of stellar sub-populations (age and abundance distributions). We discuss a radial extension of the disc evolution model representing an inside-out growth of the thin disc with constant thickness. Based on metallicity distributions of APOGEE red clump stars we derive the AMR as function of galactrocentric distance and show that mono-abundance as well as mono-age populations are flaring. The predictions of the JJ-model are consistent with the TGAS-RAVE data, which provide a significant improvement of the kinematic data and unbiased distances for more than 250,000 stars.

Keywords

Galaxy: diskGalaxy: kinematics and dynamicsGalaxy: evolutionGalaxy: solar neighbourhoodGalaxy: abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S330: Astrometry and Astrophysics in the Gaia sky , April 2017 , pp. 168 - 171
Copyright
Copyright © International Astronomical Union 2018 

References

Czekaj, M. A., Robin, A. C., Figueras, F., Luri, X., & Haywood, M., 2014, A&A, 564, A102 Google Scholar
Gaia Collaboration, Brown, A. G. A., Vallenari, A., Prusti, T., de Bruijne, J. H. J., Mignard, F., et al. 2016, A&A, 595, A2 Google Scholar
Gao, S., Just, A., & Grebel, E. K., 2013, A&A, 549, A20 Google Scholar
Green, G. M., Schlafly, E. F., Finkbeiner, D. P., et al. 2015, ApJ, 810, 25 Google Scholar
Golubov, O., Just, A., Bienaymé, O., et al. 2013, A&A, 557, A92 Google Scholar
Just, A., Gao, S. & Vidrih, S., 2011, MNRAS, 411, 2586 Google Scholar
Just, A. & Jahreiß, H., 2010, MNRAS, 402, 461 Google Scholar
Koutsouridou, I. 2017, Master thesis, Ruprecht Karls Universität, HeidelbergGoogle Scholar
Kunder, A., Kordopatis, G., Steinmetz, M., et al. 2017, ApJ, 153, 75 Google Scholar
Rybizki, J. & Just, A. 2015 MNRAS, 447, 3880 Google Scholar