The nature of CR7 revealed with MUSE: a young starburst powering extended Ly emission at z = 6.6

Author(s):: Matthee, J.; Pezzulli, G.; Mackenzie, R.; Cantalupo, S.; Kusakabe, H.; Leclercq, F.; Sobral, D.; Richard, J.; Wisotzki, L.; Lilly, S.; Boogaard, L.A. (0000-0002-3952-8588); Marino, R.; Maseda, M.V. (0000-0003-0695-4414); Nanayakkara, W.T.T. (0000-0003-2804-0648)

Published: 2020
Publication type: Article / Letter to editor

Date issued: 2020-08-22
Language: English
Is part of: Monthly Notices of the Royal Astronomical Society (2020), Vol. 498, no. 2, p. 3043-3059
hdl: 1887/3134226
doi: 10.1093/mnras/staa2550
URL: https://ui.adsabs.harvard.edu/abs/2020MNRAS.498.3043M