activity
19932023
most citedLocal Kinematics and the Local Standard of Rest

1.9k citations · 19.3k across the 178 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.GA2019★ 19 cited

Angle-action variables for orbits trapped at a Lindblad resonance

James Binney

The conventional approach to orbit trapping at Lindblad resonances via a pendulum equation fails when the parent of the trapped orbits is too circular. The problem is explained and…

astro-ph.GA2019★ 63 cited

Trapped orbits and solar-neighbourhood kinematics

James Binney

Torus mapping yields constants of motion for stars trapped at a resonance. Each such constant of motion yields a system of contours in velocity space at the Sun and neighbouring po…

astro-ph.GA2019★ 4 cited

Modelling our Galaxy

James Binney

Dynamical models will be key to exploitation of the incoming flood data for our Galaxy. Modelling techniques are reviewed with an emphasis on f(J) modelling.

astro-ph.GA2019

Flattened stellar systems based on distribution functions depending on actions

Raffaele Pascale, James Binney, Carlo Nipoti

We address an issue that arises when self-consistently flattened dynamical stellar systems are constructed by adopting a distribution function (DF) that depends on the action integ…

astro-ph.GA2019★ 29 cited

The shearing sheet and swing amplification revisited

James Binney

The principal results of the classic analysis of the shearing sheet and swing amplification by Julian & Toomre (1966) are re-derived in a more accessible way and then used to gain…

astro-ph.GA2019★ 16 cited

Relaxation of spherical stellar systems

Jun Yan Lau, James Binney

10,000 simulations of 1000-particle realisations of the same cluster are computed by direct force summation. Over three crossing times the original Poisson noise is amplified more…

astro-ph.GA2019★ 21 cited

Action-based models for dwarf spheroidal galaxies and globular clusters

Raffaele Pascale, James Binney, Carlo Nipoti +1

A new family of self-consistent DF-based models of stellar systems is explored. The stellar component of the models is described by a distribution function (DF) depending on the ac…