Use of large optical telescopes at infrared wavelengths

Details Use of large optical telescopes at infrared wavelengths Use of large optical telescopes at infrared wavelengths

Jul 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974rpnl.conf...57b&link_type=abstract

In European Southern Obs. Res. Programmes for the New Large Telescopes p 57-70 (SEE N75-15523 06-89)

Astronomy and Astrophysics

Astronomy

Infrared Spectroscopy, Infrared Stars, Telescopes, Astronomical Spectroscopy, Crab Nebula, Cygnus Constellation, High Resolution, Pulsars, Radio Galaxies, X Ray Astronomy

Scientific paper

The advantage of using large telescopes for certain infrared observations lies in their high spatial and spectral resolution. Infrared observations of extragalactic sources of centers of star formation, and of the Crab nebulae pulsar are cited as characteristic high resolution examples. Simultaneous application of X-ray, infrared, and radio source detection have made it possible to resolve fine structure, as for the 2.2 mu flare in Cyg X-3.

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