Copernicus spectra of β Lyrae

Physics

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Scientific paper

WE have observed the far ultraviolet spectrum of β Lyrae using the Princeton spectrometer, on the Copernicus satellite1. The principal data were scans in the low resolution mode (0.2 Å in the (U2) region 1,000-1,500 Å and 0.4 Å in the (V2) region 2,000-2,900 Å) at phases nearly coincident with the two light minima. Shorter scans (1,100-1,300 Å) were obtained at the two quadrature phases. All observations were made in August and September 1973 but not in the same orbital cycle.

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