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General spherical anisotropic Jeans models of stellar kinematics: including proper motions and radial velocities

Abstract:
Cappellari (2008) presented a flexible and efficient method to model the stellar kinematics of anisotropic axisymmetric and spherical stellar systems. The spherical formalism could be used to model the line-of-sight velocity second moments allowing for essentially arbitrary radial variations in the anisotropy and general luminous and total density profiles. Here we generalize the spherical formalism by providing the expressions for all three components of the projected second moments, including the two proper motion components. A reference implementation is now included in the public JAM package available at http://purl.org/cappellari/software.
Publication status:
Not published
Peer review status:
Not peer reviewed

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author


Publication date:
2015-05-01


Keywords:
Pubs id:
pubs:673593
UUID:
uuid:9c6bff0b-9722-4253-99b4-698e78b26438
Local pid:
pubs:673593
Source identifiers:
673593
Deposit date:
2017-01-30

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