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:

The MUSE Ultra Deep Field (MUDF). I : discovery of a group of Lyα nebulae associated with a bright z ≈ 3.23 quasar pair.

Lusso, E. and Fumagalli, M. and Fossati, M. and Mackenzie, R. and Bielby, R. M. and Battaia, F. Arrigoni and Cantalupo, S. and Cooke, R. and Cristiani, S. and Dayal, P. and D’Odorico, V. and Haardt, F. and Lofthouse, E. and Morris, S. and Peroux, C. and Prichard, L. and Rafelski, M. and Simcoe, R. and Swinbank, M. and Theuns, T. (2019) 'The MUSE Ultra Deep Field (MUDF). I : discovery of a group of Lyα nebulae associated with a bright z ≈ 3.23 quasar pair.', Monthly notices of the Royal Astronomical Society : letters., 485 (1). L62-L67.

Abstract

We present first results from Multi Unit Spectroscopic Explorer (MUSE) observations at the Very Large Telescope in the MUSE Ultra Deep Field (MUDF), a ≈1.2 × 1.4 arcmin2 region for which we are collecting ≈200 hours of integral field spectroscopy. The ≈40-h observation completed to date reveals the presence of a group of three Lyα nebulae associated with a bright quasar pair at z ≃ 3.23 with projected separation of ≈500 kpc⁠. Two of the nebulae are physically associated with the quasars which are likely powering the Lyα emission, and extend for ≳100 kpc at a surface brightness level of ≈6 × 10−19 ergs−1cm−2arcsec−2⁠. A third smaller (≈35 kpc) nebula lies at a velocity offset of ≈1550 km s−1. Despite their clustered nature, the two large nebulae have properties similar to those observed in isolated quasars and exhibit no sharp decline in flux at the current depth, suggesting an even more extended distribution of gas around the quasars. We interpret the shape and the alignment of the two brighter nebulae as suggestive of the presence of an extended structure connecting the two quasar host galaxies, as seen for massive galaxies forming within gas-rich filaments in cosmological simulations.

Item Type:Article
Full text:(VoR) Version of Record
Download PDF
(2224Kb)
Status:Peer-reviewed
Publisher Web site:https://doi.org/10.1093/mnrasl/slz032
Publisher statement:© 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
Date accepted:01 March 2019
Date deposited:28 March 2019
Date of first online publication:07 March 2019
Date first made open access:28 March 2019

Save or Share this output

Export:
Export
Look up in GoogleScholar