Optical and Ultraviolet Spectroscopy of the Nuclei of Seyfert Galaxies

Details Optical and Ultraviolet Spectroscopy of the Nuclei of Seyfert Galaxies Optical and Ultraviolet Spectroscopy of the Nuclei of Seyfert Galaxies

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980msngr..22...14s&link_type=abstract

The Messenger, No.22, P. 14, 1980

Physics

1

Scientific paper

The launching of the International Ultraviolet Explorer (IUE) in 1978 has made the ultraviolet sky in the wavelength region from 1150 A to 3200 A accessible to detailed spectroscopic study. The IUE is a satellite in a geosynchronous orbit, equipped with a 45 cm telescope with two spectrographs. For a more detailed description of this satellite, the interested reader is referred to the article by A. Heck et al. (Messenger No. 15, Oec. 1978). Although the diameter of the IUE telescope is quite small-its size is more typical of an amateur telescope than of a scientific instrument-it has been used successfully even for extragalactic spectroscopy.

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