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Halo Kinematic Streams in the Era of Gaia

Published online by Cambridge University Press:  06 January 2014

Paola Re Fiorentin ,
Anna Curir ,
Mario G. Lattanzi  and
Alessandro Spagna
Paola Re Fiorentin
Affiliation:
INAF - Torino Astrophysical Observatory, strada Osservatorio 20, 10025 Pino T. se, Italy email: re_fiorentin@oato.inaf.it
Anna Curir
Affiliation:
INAF - Torino Astrophysical Observatory, strada Osservatorio 20, 10025 Pino T. se, Italy email: re_fiorentin@oato.inaf.it
Mario G. Lattanzi
Affiliation:
INAF - Torino Astrophysical Observatory, strada Osservatorio 20, 10025 Pino T. se, Italy email: re_fiorentin@oato.inaf.it
Alessandro Spagna
Affiliation:
INAF - Torino Astrophysical Observatory, strada Osservatorio 20, 10025 Pino T. se, Italy email: re_fiorentin@oato.inaf.it
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Abstract

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We report on the discovery and characterization of a possibly new signature related to the formation of the Milky Way stellar local halo.

Keywords

Galaxy: formationhalokinematics and dynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S298: Setting the scene for Gaia and LAMOST , May 2013 , pp. 434
Copyright
Copyright © International Astronomical Union 2014 

References

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Murante, G., Poglio, E., Curir, A., & Villalobos, A. 2010, ApJ, 716, L115CrossRefGoogle Scholar