Lyman-alpha imagery of comet Kohoutek, and far-UV magnitudes of stars

Astronomy and Astrophysics – Astronomy

Scientific paper

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Brightness, Far Ultraviolet Radiation, Imaging Techniques, Kohoutek Comet, Lyman Alpha Radiation, Ultraviolet Photography, Astronomical Photography, Electronography, Galaxies, Hydrogen, Magellanic Clouds, Nebulae, Skylab 4, Spaceborne Astronomy, Stellar Radiation

Scientific paper

The Apollo-16 S201 electronographic camera backup model was modified for use on the Skylab AMS-SAL, which reduced its 20 deg FOV to about 7 deg unvignetted. Over 500 frames were exposed by automatic sequencer through LiF and CaF2. The Lyman-alpha halo of comet Kohoutek has been analyzed for nine occasions, and its long, pointed tail was imaged in 1250-1600 A only near perihelion. Far-UV magnitudes and colors are being derived for about 200 stars, nebulae, and galaxies. Redshifted Lyman-alpha emission from intergalactic atomic hydrogen was not detected in 7 clusters of galaxies. About 25% of the exposed frames were degraded by water damage, electrical discharges, decline in photocathode sensitivity, and loss of AMS mirror reflectance.

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