Line identifications in the ultraviolet spectrum of Gamma Pegasi (B2 IV)

Details Line identifications in the ultraviolet spectrum of Gamma Pegasi (B2 IV) Line identifications in the ultraviolet spectrum of Gamma Pegasi (B2 IV)

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apjs...37..265h&link_type=abstract

Astrophysical Journal Supplement Series, vol. 37, June 1978, p. 265-286.

Astronomy and Astrophysics

Astronomy

4

Early Stars, Line Spectra, Stellar Spectrophotometry, Ultraviolet Spectra, Abundance, Atomic Spectra, Oao 3, Ultraviolet Astronomy

Scientific paper

UV tracings made from the Copernicus satellite of Gamma Pegasi (B2 IV) are examined in terms of element abundance, including the following: H I, He I, C II, C III, N I, N II, N III, O II, Mg II, Si II, P IV, S IV, Cl II, Cr II, Mn II, Ni III, and Fe II. The U2 spectrometer covered wavelengths from double lambda 1000-1448 at a resolution of 0.2A, while the V2 spectrometer covered wavelengths from double lambda 2000-3000 at a resolution of 0.4 A. Comparisons are made between these data and identification studies of three other early- and mid-B stars, also using Copernicus observations.

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