Schwarzschild dynamical model of the Fornax dwarf spheroidal galaxy

Klaudia Kowalczyk; Andrés del Pino; Ewa L. Lokas; Monica Valluri

doi:10.1093/mnras/sty3100

paper

Schwarzschild dynamical model of the Fornax dwarf spheroidal galaxy

arXiv:1807.07852 · doi:10.1093/mnras/sty3100

Abstract

We present a full dynamical model of the Fornax dwarf spheroidal galaxy obtained with the spherically symmetric Schwarzschild orbit superposition method applied to the largest kinematic data set presently available. We modelled the total mass content of the dwarf with the mass-to-light ratio $Υ$ varying with radius and found that Fornax is with high probability embedded in a massive and extended dark matter halo. We estimated the total mass contained within 1kpc to be $M (< 1$ kpc $) = 1.2 5_{- 0.13}^{+ 0.06} \times 1 0^{8}$ M $_{⊙}$ . The data are consistent with the constant mass-to-light ratio, i.e. the mass-follows-light model, only at 3 $σ$ level, but still require a high value of $Υ \approx 11.2$ M $_{⊙} /$ L $_{⊙}$ . Our results are in general agreement with previous estimates of the dynamical mass profile of Fornax. As the Schwarzschild method does not require any assumptions on the orbital anisotropy of the stars, we obtained a profile of the anisotropy parameter $β$ as an output of our modelling. The derived anisotropy is close to zero in the centre of the galaxy and decreases with radius, but remains consistent with isotropic orbits at all radii at 1 $σ$ confidence level.

arXiv comment11 pages, 9 figures, 3 tables, accepted for publication in MNRAS

Schwarzschild dynamical model of the Fornax dwarf spheroidal galaxy

Abstract

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