The Copernicus ultraviolet spectral atlas of Beta Orionis

Details The Copernicus ultraviolet spectral atlas of Beta Orionis The Copernicus ultraviolet spectral atlas of Beta Orionis

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apjs...49..353r&link_type=abstract

Astrophysical Journal Supplement Series, vol. 49, July 1982, p. 353-404.

Astronomy and Astrophysics

Astronomy

11

B Stars, Graphs (Charts), Stellar Spectra, Supergiant Stars, Ultraviolet Astronomy, High Resolution, Light Scattering, Line Spectra, Oao 3, Wavelengths

Scientific paper

An ultraviolet spectral atlas is presented for the B8 Ia star Beta Orionis, which has been scanned from 999 to 1561 A by the Princeton spectrometer aboard the Copernicus satellite. From 999 to 1420 A the observations have a nominal resolution of 0.05 A. At the longer wavelengths the resolution is 0.1 A. The atlas is presented in graphs. Lines identified in the spectrum are also listed.

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