ultraviolet astronomy

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ultraviolet astronomy

n.
The branch of astronomy that uses observations of emissions in the ultraviolet part of electromagnetic spectrum to study extraterrestrial sources such as stars, planets, galaxies, and interstellar gas clouds.
American Heritage® Dictionary of the English Language, Fifth Edition. Copyright © 2016 by Houghton Mifflin Harcourt Publishing Company. Published by Houghton Mifflin Harcourt Publishing Company. All rights reserved.

ultraviolet astronomy

n
(Astronomy) the study of radiation from celestial sources in the wavelength range 91.2 to 320 nanometres, 12 to 91.2 nanometres being the extreme ultraviolet range
Collins English Dictionary – Complete and Unabridged, 12th Edition 2014 © HarperCollins Publishers 1991, 1994, 1998, 2000, 2003, 2006, 2007, 2009, 2011, 2014
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References in periodicals archive
FUSE specializes in the ultraviolet wavebands between those of the Hubble Space Telescope and the Extreme Ultraviolet Explorer. It carries high- resolution spectrographs to study emission and absorption lines in stars, galaxies, and the interstellar medium.
Recording the emission and absorption of ultraviolet light with wavelengths from 90 to 120 nanometers, FUSE will fill the gap between the Hubble Space Telescope, which detects only the near ultraviolet, and the Extreme Ultraviolet Explorer.
Since its launch in June 1992, the Extreme Ultraviolet Explorer satellite has opened a wide window on a largely unexplored slice of the electromagnetic spectrum.
And we did just that, since we were lucky enough to observe Nova Cygni 1992 with Voyager 2, the Extreme Ultraviolet Explorer (EUVE), and the Rosat X-ray satellite.
The ROSAT and Extreme Ultraviolet Explorer satellites have since revealed that Hyakutake is not alone--at least 10 comets, including Hale-Bopp, are now known to exhibit an X-ray glow as they near the sun.
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