Kinematic deprojection and mass inversion of spherical systems of known velocity anisotropy
arXiv:0906.4971 · doi:10.1111/j.1365-2966.2009.15817.x
Abstract
Traditionally, the mass / velocity anisotropy degeneracy (MAD) inherent in the spherical, stationary, non-streaming Jeans equation has been handled by assuming a mass profile and fitting models to the observed kinematical data. Here, the opposite approach is considered: the equation of anisotropic kinematic projection is inverted for known arbitrary anisotropy to yield the space radial velocity dispersion profile in terms of an integral involving the radial profiles of anisotropy and isotropic dynamical pressure. Then, through the Jeans equation, the mass profile is derived in terms of double integrals of observable quantities. Single integral formulas for both deprojection and mass inversion are provided for several simple anisotropy models (isotropic, radial, circular, general constant, Osipkov-Merritt, Mamon-Lokas and Diemand-Moore-Stadel). Tests of the mass inversion on NFW models with these anisotropy models yield accurate results in the case of perfect observational data, and typically better than 70% (in 4 cases out of 5) accurate mass profiles for the sampling errors expected from current observational data on clusters of galaxies. For the NFW model with mildly increasing radial anisotropy, the mass is found to be insensitive to the adopted anisotropy profile at 7 scale radii and to the adopted anisotropy radius at 3 scale radii. This anisotropic mass inversion method is a useful complementary tool to analyze the mass and anisotropy profiles of spherical systems. It provides the practical means to lift the MAD in quasi-spherical systems such as globular clusters, round dwarf spheroidal and elliptical galaxies, as well as groups and clusters of galaxies, when the anisotropy of the tracer is expected to be linearly related to the slope of its density.
Accepted in MNRAS. 19 pages. Minor changes from previous version: Table 1 of nomenclature, some math simplifications, paragraph in Discussion on alternative deprojection method by deconvolution. 19 pages. 6 figures
References in corpus (7)
- Accurate masses for dispersion-supported galaxies
- A universal density slope - velocity anisotropy relation for relaxed structures
- NMAGIC: Fast Parallel Implementation of a Chi-Squared-Made-to-Measure Algorithm for Modelling Observational Data
- Velocity dispersion around ellipticals in MOND
- The distribution function of dark matter in massive haloes
- The dynamical structure of dark matter haloes
- Circular velocity profiles of dark matter haloes
Cited by in corpus (39)
- Accurate masses for dispersion-supported galaxies
- Galaxy Masses
- The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
- MAMPOSSt: Modelling Anisotropy and Mass Profiles of Observed Spherical Systems. I. Gaussian 3D velocities
- The universal distribution of halo interlopers in projected phase space. Bias in galaxy cluster concentration and velocity anisotropy?
- The effect of baryons on the inner density profiles of rich clusters
- NGC6240: Merger-Induced Star Formation & Gas Dynamics
- Mass profiles and galaxy orbits in nearby galaxy clusters from the analysis of the projected phase-space
- The GOGREEN survey: The environmental dependence of the star-forming galaxy main sequence at
- A critical reassessment of particle Dark Matter limits from dwarf satellites
- Structural and dynamical modeling of WINGS clusters. II. The orbital anisotropies of elliptical, spiral and lenticular galaxies
- Jeans modelling of the Milky Way's nuclear stellar disc
- A new method to measure the mass of galaxy clusters
- Dynamical Models of Elliptical Galaxies -- I. Simple Methods
- Stellar graveyards: Clustering of compact objects in globular clusters NGC 3201 and NGC 6397
- Bridging the gap between low and high mass dwarf galaxies
- Model-independent X-ray mass determinations
- N-body simulations of the Carina dSph in MOND
- Dynamical signatures of infall around galaxy clusters: a generalized Jeans equation
- GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ()
- Dark Matter Density Profiles in Dwarf Galaxies: Linking Jeans Modeling Systematics and Observation
- A novel JEAnS analysis of the Fornax dwarf using evolutionary algorithms: mass follows light with signs of an off-centre merger
- An accurate analytic mass model for lensing galaxies
- An attractor for dark matter structures
- Dynamical analysis of clusters of galaxies from cosmological simulations
- The projected gravitational potential of the galaxy cluster MACS~J1206 derived from galaxy kinematics
- Testing a simple recipe for estimating galaxy masses from minimal observational data
- Reconstructing the projected gravitational potential of galaxy clusters from galaxy kinematics
- Combining Strong Lensing and Dynamics in Galaxy Clusters: integrating MAMPOSSt within LENSTOOL I. Application on SL2S J02140-0535
- Reliable mass calculation in spherical gravitating systems
- Constraints on velocity anisotropy of spherical systems with separable augmented densities
- SpheCow: flexible dynamical models for galaxies and dark matter haloes
- Dynamics of dwarf galaxies in gravity
- Challenges in modeling the dark matter halo of NGC 1052-DF2: Cored versus cuspy halo models
- Weak lensing reconstructions in 2D & 3D: implications for cluster studies
- Boosting the evolutionary picture of Cl 0024+17 and MS 0451-03: A case study at intermediate-redshift
- Dynamics of Dwarf Galaxies in Scalar-Tensor-Vector-Gravity
- Dynamical Properties and Velocity Dispersion-Mass Relation of Galaxy Clusters from the GOGREEN and GCLASS Surveys
- X-ray emission of the Nuclear Stellar Disk as seen by SRG/ART-XC