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The asymmetric drift, the local standard of rest, and implications from RAVE data

2013/07/23 by O. Golubov, Oleksiy Golubov, A. Just +20 · 2 citations
Mathematics · Physics and Astronomy · #Astro and Planetary Science #Astrophysics #Classical mechanics #Context (archaeology) #Geodesy #Geography #Mathematics #Motion (physics) #Physics #Proper motion #Rest (music) #Solar and Space Plasma Dynamics #Stars #Statistics #Stellar, planetary, and galactic studies #Value (mathematics) #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201321559

Accepted for publication in A&A; 13 pages, 9 figures

arxiv created 2013/07/23 · openalex publication_date 2013/07/23 · arxiv updated 2015/06/16 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06

Abstract

Context. The determination of the local standard of rest (LSR), which corresponds to the measurement of the peculiar motion of the Sun based on the derivation of the asymmetric drift of stellar populations, is still a matter of debate. The classical value of the tangential peculiar motion of the Sun with respect to the LSR was challenged in recent years, claiming a significantly larger value.

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