University of Surrey

Test tubes in the lab Research in the ATI Dance Research

A semi-analytic dynamical friction model for cored galaxies

Petts, James, Read, Justin and Gualandris, Alessia (2016) A semi-analytic dynamical friction model for cored galaxies Monthly Notices of the Royal Astronomical Society, 463 (1). pp. 858-869.

[img]
Preview
Text
MNRAS-2016-Petts-mnras_stw2011.pdf - Accepted version Manuscript
Available under License : See the attached licence file.

Download (907kB) | Preview
[img]
Preview
Text (licence)
SRI_deposit_agreement.pdf
Available under License : See the attached licence file.

Download (33kB) | Preview

Abstract

We present a dynamical friction model based on Chandrasekhar’s formula that reproduces the fast inspiral and stalling experienced by satellites orbiting galaxies with a large constant density core. We show that the fast inspiral phase does not owe to resonance. Rather, it owes to the background velocity distribution function for the constant density core being dissimilar from the usually-assumed Maxwellian distribution. Using the correct background velocity distribution function and the semi-analytic model from Petts, Gualandris & Read (2015), we are able to correctly reproduce the infall rate in both cored and cusped potentials. However, in the case of large cores, our model is no longer able to correctly capture core-stalling. We show that this stalling owes to the tidal radius of the satellite approaching the size of the core. By switching off dynamical friction when rt(r) = r (where rt is the tidal radius at the satellite’s position) we arrive at a model which reproduces the N-body results remarkably well. Since the tidal radius can be very large for constant density background distributions, our model recovers the result that stalling can occur for Ms/Menc 1, where Ms and Menc are the mass of the satellite and the enclosed galaxy mass, respectively. Finally, we include the contribution to dynamical friction that comes from stars moving faster than the satellite. This next-to-leading order effect becomes the dominant driver of inspiral near the core region, prior to stalling.

Item Type: Article
Subjects : Physics
Divisions : Faculty of Engineering and Physical Sciences > Physics
Authors :
NameEmailORCID
Petts, Jamesj.petts@surrey.ac.ukUNSPECIFIED
Read, Justinj.read@surrey.ac.ukUNSPECIFIED
Gualandris, Alessiaa.gualandris@surrey.ac.ukUNSPECIFIED
Date : 12 August 2016
Identification Number : 10.1093/mnras/stw2011
Copyright Disclaimer : 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society
Uncontrolled Keywords : Galaxies: kinematics and dynamics – Galaxies: star clusters – methods: numerical.
Related URLs :
Depositing User : Symplectic Elements
Date Deposited : 09 Sep 2016 11:04
Last Modified : 04 Aug 2017 17:39
URI: http://epubs.surrey.ac.uk/id/eprint/812068

Actions (login required)

View Item View Item

Downloads

Downloads per month over past year


Information about this web site

© The University of Surrey, Guildford, Surrey, GU2 7XH, United Kingdom.
+44 (0)1483 300800