The Copernicus ultraviolet spectral atlas of Gamma Pegasi

Details The Copernicus ultraviolet spectral atlas of Gamma Pegasi The Copernicus ultraviolet spectral atlas of Gamma Pegasi

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apjs...57..751r&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 57, April 1985, p. 751-822.

Astronomy and Astrophysics

Astrophysics

11

B Stars, Early Stars, Oao 3, Satellite Observation, Stellar Spectra, Ultraviolet Spectra, Abundance, Astronomical Spectroscopy, Light Scattering, Line Spectra, Spectral Resolution, Tables (Data)

Scientific paper

An ultraviolet spectral atlas is presented for the B2 IV star γ Pegasi, which has been scanned from 970 to 1501 Å by the Princeton spectrometer aboard the Copernicus satellite. From 970 to 1430 Å the observations have a nominal resolution of 0.05 Å. At the longer wavelengths the resolution is 0.1 Å. The atlas is presented in graphs. Line identifications are also listed.

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