Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

Fluorescent rings in star-free dark matter haloes.

Sykes, Calvin and Fumagalli, Michele and Cooke, Ryan and Theuns, Tom and Benítez–Llambay, Alejandro (2019) 'Fluorescent rings in star-free dark matter haloes.', Monthly notices of the Royal Astronomical Society., 487 (1). pp. 609-621.

Abstract

Photoheating of the gas in low-mass dark matter (DM) haloes prevents baryons from cooling, leaving the haloes free of stars. Gas in these ‘dark’ haloes remains exposed to the ultraviolet background (UVB), and so is expected to emit via fluorescent recombination lines. We present a set of radiative transfer simulations, which model dark haloes as spherical gas clouds in hydrostatic equilibrium with a DM halo potential, and in thermal equilibrium with the UVB at redshift z = 0. We use these simulations to predict surface brightnesses in Hα, which we show to have a characteristic ring-shaped morphology for haloes in a narrow mass range between ≃ 109.5 and 109.6 M⊙. We explore how this emission depends on physical parameters such as the DM density profile and the UVB spectrum. We predict the abundance of fluorescent haloes on the sky, and discuss possible strategies for their detection. We demonstrate how detailed observations of fluorescent rings can be used to infer the properties of the haloes which host them, such as their density profiles and the mass-concentration relation, as well as to directly measure the UVB amplitude.

Item Type:Article
Full text:(AM) Accepted Manuscript
Download PDF
(836Kb)
Full text:(VoR) Version of Record
Download PDF
(2532Kb)
Status:Peer-reviewed
Publisher Web site:https://doi.org/10.1093/mnras/stz1234
Publisher statement:© 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
Date accepted:22 April 2019
Date deposited:07 May 2019
Date of first online publication:04 May 2019
Date first made open access:No date available

Save or Share this output

Export:
Export
Look up in GoogleScholar