A Metal-poor Damped Ly α System at Redshift 6.4
© 2019. The American Astronomical Society. All rights reserved. We identify a strong Lyα damping wing profile in the spectrum of the quasar P183+05 at z = 6.4386. Given the detection of several narrow metal absorption lines at z = 6.40392, the most likely explanation for the absorption profile is th...
Main Authors: | , , , , , , , , , , , , |
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Format: | Article |
Language: | English |
Published: |
American Astronomical Society
2021
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Online Access: | https://hdl.handle.net/1721.1/132356 |