Calculation of the Local Standard of Rest from 20,574 Local Stars in the New Hipparcos Reduction with Known Radial Velocities
Charles Francis, Erik Anderson

TL;DR
This paper accurately estimates the local standard of rest (LSR) using a large sample of nearby stars, addressing limitations of traditional methods by considering the structured velocity distribution, and provides refined values for Galactic parameters.
Contribution
It introduces an alternative approach to calculating the LSR that accounts for velocity distribution structure, improving accuracy over traditional mean-based methods.
Findings
Best estimate of LSR: (7.5, 13.5, 6.8) km/s with errors
Circular speed curve slope at solar radius: -9.3 km/s/kpc
Traditional methods fail due to velocity distribution structure
Abstract
Context. An accurate estimate of the local standard of rest (LSR) is required to determine key parameters used in approximate galactic mass models and to understand Galactic structure and evolution. However, authors are often forced to base dynamical analyses on potentially unreliable figures because recent determinations of the LSR have failed to reach agreement, especially with regard to the direction, V, of Galactic rotation. Aims. To explain why the traditional method for calculating the LSR fails, and to find alternative means of calculating the LSR with realistic error margins. Methods. We assemble and investigate the kinematic properties of 20 574 stars within 300pc, with complete and accurate kinematic data. The traditional method of calculating the LSR assumes a well-mixed distribution. In fact, the velocity distribution is highly structured, invalidating calculations based on…
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