Future prospects for spectroscopic and direct work - Optical and UV

Details Future prospects for spectroscopic and direct work - Optical and UV Future prospects for spectroscopic and direct work - Optical and UV

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978phys...17..321b&link_type=abstract

(Niels Bohr Institut, Teknisk Videnskabelige Forskningsrad, and Nordisk Institut for Teoretisk Atomfysik, Symposium on Quasars a

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Hubble Space Telescope, Spaceborne Astronomy, Ultraviolet Astronomy, Angular Resolution, Cosmology, Galactic Nuclei, Galactic Structure, Line Spectra, Quasars, Seyfert Galaxies, Technology Utilization

Scientific paper

A description of the main features and proposed instrumentation of the 2.4 m Space Telescope is given. Highlights of work that can be planned on active nuclei of galaxies, QSOs, and BL Lac objects are briefly outlined, involving spectroscopy over wavelengths from 1200 A to 1 mm, direct imaging with 0.1 sec resolution, and the capability for 0.1 sec resolution along the spectrograph slit. The resolution, the much reduced sky background, and the full wavelength coverage also make possible important observations relevant to cosmology.

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