The absolute flux of six hot stars in the ultraviolet (912-1600 A)

Details The absolute flux of six hot stars in the ultraviolet (912-1600 A) The absolute flux of six hot stars in the ultraviolet (912-1600 A)

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...292..676w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 292, May 15, 1985, p. 676-686.

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19

Hot Stars, Stellar Radiation, Stellar Spectra, Ultraviolet Spectra, Early Stars, Flux Density, Stellar Spectrophotometry, Voyager 1 Spacecraft, Voyager 2 Spacecraft

Scientific paper

Six hot stars were observed on 1984 March 2 from a Black Brant V sounding rocket (NASA 21.085UG). The absolute fluxes from Gamma 2 Vel, Zeta Pup, Alpha CMa ,Gamma Ori, Beta Tau, and Epsilon Per were measured in the spectral region between 912 and 1600 A at 10 A resolution. Comparisons with revised Voyager 1 and Voyager 2 Ultraviolet Spectrometer data and previous sounding rocket data are evaluated. In general, the two sounding rocket experiments are in good agreement, and the revised Voyager data and the sounding rocket data are in agreement except at wavelengths below 1000 A.

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