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We present spatially resolved Ly\u2009\u03b1 spectroscopy with VLT\/MUSE targeting VR7, a UV-luminous galaxy at z\u00a0= 6.532 with moderate Ly\u2009\u03b1 equivalent width (EW0\u00a0\u2248\u00a038\u2009\u00c5). These data are combined with deep resolved [CII]158\u03bcm spectroscopy obtained with ALMA and UV imaging from HST and we also detect UV continuum with MUSE. Ly\u2009\u03b1 emission is clearly detected with S\/N\u00a0\u2248\u00a040 and FWHM of 374\u2009km\u2009s\u22121. Ly\u2009\u03b1 and [C\u2009ii] are similarly extended beyond the UV, with effective radius reff\u00a0= 2.1\u00a0\u00b1\u00a00.2\u2009kpc for a single exponential model or r$_{\\rm eff, Ly\\alpha , halo} = 3.45^{+1.08}_{-0.87}$ kpc when measured jointly with the UV continuum. The Ly\u2009\u03b1 profile is broader and redshifted with respect to the [C\u2009ii] line (by 213\u2009km\u2009s\u22121), but there are spatial variations that are qualitatively similar in both lines and coincide with resolved UV components. This suggests that the emission originates from two components with plausibly different H\u2009i column densities. We place VR7 in the context of other galaxies at similar and lower redshift. The Ly\u2009\u03b1 halo scale length is similar at different redshifts and velocity shifts with respect to the systemic are typically smaller. Overall, we find little indications of a more neutral vicinity at higher redshift. This means that the local (\u223c10\u2009kpc) neutral gas conditions that determine the observed Ly\u2009\u03b1 properties in VR7 resemble the conditions in post-reionization galaxies.<\/jats:p>","DOI":"10.1093\/mnras\/stz3554","type":"journal-article","created":{"date-parts":[[2019,12,19]],"date-time":"2019-12-19T04:35:19Z","timestamp":1576730119000},"page":"1778-1790","source":"Crossref","is-referenced-by-count":21,"title":["Resolved Lyman-\u03b1 properties of a luminous Lyman-break galaxy in a large ionized bubble at <i>z<\/i>\u00a0= 6.53"],"prefix":"10.1093","volume":"492","author":[{"ORCID":"https:\/\/orcid.org\/0000-0003-2871-127X","authenticated-orcid":false,"given":"Jorryt","family":"Matthee","sequence":"first","affiliation":[{"name":"Department of Physics, ETH Z\u00fcrich, Wolfgang-Pauli-Strasse 27, CH-8093 Z\u00fcrich, Switzerland"}]},{"given":"David","family":"Sobral","sequence":"additional","affiliation":[{"name":"Department of Physics, Lancaster University, Lancaster LA1 4YB, UK"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-2491-060X","authenticated-orcid":false,"given":"Max","family":"Gronke","sequence":"additional","affiliation":[{"name":"Department of Physics and Astronomy, University of California, Santa Barbara, CA 93106, USA"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-0736-7879","authenticated-orcid":false,"given":"Gabriele","family":"Pezzulli","sequence":"additional","affiliation":[{"name":"Department of Physics, ETH Z\u00fcrich, Wolfgang-Pauli-Strasse 27, CH-8093 Z\u00fcrich, Switzerland"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-5804-1428","authenticated-orcid":false,"given":"Sebastiano","family":"Cantalupo","sequence":"additional","affiliation":[{"name":"Department of Physics, ETH Z\u00fcrich, Wolfgang-Pauli-Strasse 27, CH-8093 Z\u00fcrich, Switzerland"}]},{"given":"Huub","family":"R\u00f6ttgering","sequence":"additional","affiliation":[{"name":"Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Netherlands"}]},{"given":"Behnam","family":"Darvish","sequence":"additional","affiliation":[{"name":"Cahill Center for Astrophysics, California Institute of Technology, 1216 East California Boulevard, Pasadena, CA 91125, USA"}]},{"given":"S\u00e9rgio","family":"Santos","sequence":"additional","affiliation":[{"name":"Department of Physics, Lancaster University, Lancaster LA1 4YB, UK"}]}],"member":"286","published-online":{"date-parts":[[2019,12,20]]},"reference":[{"key":"2020121920091952500_bib1","doi-asserted-by":"publisher","first-page":"922","DOI":"10.1086\/338497","volume":"567","author":"Ahn","year":"2002","journal-title":"ApJ"},{"key":"2020121920091952500_bib2","doi-asserted-by":"publisher","first-page":"A33","DOI":"10.1051\/0004-6361\/201322068","volume":"558","author":"Astropy Collaboration","year":"2013","journal-title":"A&A"},{"key":"2020121920091952500_bib3","doi-asserted-by":"crossref","first-page":"773508","DOI":"10.1117\/12.856027","volume-title":"Ground-based and Airborne Instrumentation for Astronomy III","author":"Bacon","year":"2010"},{"key":"2020121920091952500_bib4","doi-asserted-by":"publisher","first-page":"A1","DOI":"10.1051\/0004-6361\/201730833","volume":"608","author":"Bacon","year":"2017","journal-title":"A&A"},{"key":"2020121920091952500_bib5","doi-asserted-by":"publisher","first-page":"473","DOI":"10.1038\/nature25180","volume":"553","author":"Ba\u00f1ados","year":"2018","journal-title":"Nature"},{"key":"2020121920091952500_bib6","doi-asserted-by":"publisher","first-page":"1723","DOI":"10.1111\/j.1365-2966.2011.18789.x","volume":"416","author":"Barnes","year":"2011","journal-title":"MNRAS"},{"key":"2020121920091952500_bib7","first-page":"112","volume-title":"ASP Conf. 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