Far Ultra-violet Spectra of Orion Stars

Details Far Ultra-violet Spectra of Orion Stars Far Ultra-violet Spectra of Orion Stars

Sep 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967natur.215.1257j&link_type=abstract

Nature, Volume 215, Issue 5107, pp. 1257-1259 (1967).

Physics

26

Scientific paper

FAR ULTRA-VIOLET spectra of the brighter stars in the vicinity of ɛ Orionis were photographed with an objective spectrograph carried to 165 km by an Aerobee 150 rocket launched from the White Sands Missile Range on September 20, 1966, at 10h 45m U.T. As with previous Princeton flights1,2 the spectrograph was stabilized by a passive gyro system which limited angular motion in the dispersion direction to about +/-20'' during a 3 min exposure giving a resolution of about 1 Å.

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