Blue spectrum of subdwarf G27-44

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Дата индексирования: Mon Oct 1 22:19:32 2012
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High resolution (R=60000) spectrum of the metal poor star G27-44 in the spectral region 3500-5000 AA was obtained by S.Ermakov, V.Klochkova and V.Panchuk with the echelle spectrometer NES BTA on July, 2001.
The most strong absorbtions are H, K CaII lines.

High resolution (R=60000) spectrum of the metal poor star G27-44 in the spectral region 3500-5000 AA was obtained by S.Ermakov, V.Klochkova and V.Panchuk with the echelle spectrometer NES BTA on July, 2001. The most strong absorbtions are H, K CaII lines.

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High resolution (R=60000) spectrum of the metal poor star G27-44 in the spectral region 3500-5000 AA was obtained by S.Ermakov, V.Klochkova and V.Panchuk with the echelle spectrometer NES BTA on July, 2001.
The most strong absorbtions are H, K CaII lines.