Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12666/157
Title: An ionized superbubble powered by a protocluster at z = 6.5
Authors: Rodríguez Espinosa, J. M.
Mas Hesse, J. M.
Salvador Solé, E.
Calvi, R.
Manrqiue, A.
Chanchaiworawit, K.
Guzman, R.
Gallego, J.
Herrero, A.
Marín Franch, A.
Keywords: Galaxies: high redshift;Galaxies; star formation;Cosmology: reionization;Cosmology: early universe
Issue Date: 18-Mar-2020
Publisher: Oxford Academics: Oxford University Press
DOI: 10.1093/mnrasl/slaa045
Published version: https://academic.oup.com/mnrasl/article/495/1/L17/5809363
Citation: Monthly Notices of the Royal Astronomical Society: Letters 495(1): L17- L21 (2020)
Abstract: We show herein that a proto-cluster of Ly α emitting galaxies, spectroscopically confirmed at redshift 6.5, produces a remarkable number of ionizing continuum photons. We start from the Ly α fluxes measured in the spectra of the sources detected spectroscopically. From these fluxes, we derive the ionizing emissivity of continuum photons of the protocluster, which we compare with the ionizing emissivity required to reionize the protocluster volume. We find that the sources in the protocluster are capable of ionizing a large bubble, indeed larger than the volume occupied by the protocluster. For various calculations, we have used the model AMIGA, in particular to derive the emissivity of the Lyman continuum photons required to maintain the observed volume ionized. Besides, we have assumed the ionizing photons escape fraction given by AMIGA at this redshift.
URI: http://hdl.handle.net/20.500.12666/157
E-ISSN: 1745-3933
ISSN: 1745-3925
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