Hostname: page-component-cb9f654ff-kl2l2 Total loading time: 0 Render date: 2025-08-22T09:28:13.960Z Has data issue: false hasContentIssue false
  • English
  • Français

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
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.

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

References

Helmi, A., White, S. D. M., de Zeeuw, P. T., & Zhao, H. S. 1999, Nature, 402, 53Google Scholar
Kepley, A. A., Morrison, H. L., Helmi, A., et al. 2007, AJ, 134, 1579CrossRefGoogle Scholar
Murante, G., Poglio, E., Curir, A., & Villalobos, A. 2010, ApJ, 716, L115CrossRefGoogle Scholar