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Home All issues Volume 582 (October 2015) A&A, 582 (2015) A94 Full HTML
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Fig. 1

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FUSE spectrum of PG 1707+427 (thin line) compared to a photospheric model spectrum (thick line) with the finally adopted parameters as listed in Table 1. The main photospheric spectral lines are identified. Complete line lists are given in Tables 2–5. Question marks denote unidentified lines.

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