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Дата изменения: Unknown Дата индексирования: Mon Oct 1 23:29:47 2012 Кодировка: |
The same as in Fig. 1. In this wavelength range the spectral orders mostly do not overlap. This is why only two spectra from the 1-m SAO telescope show the strong 7224 DIB which is usually intertwined with a telluric line and difficult to cancel out.
<Download average spectrum of o Per>
<Download average spectrum of reddened stars>