A new small-dispersion objective prism for the Curtis telescope

Details A new small-dispersion objective prism for the Curtis telescope A new small-dispersion objective prism for the Curtis telescope

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974pasp...86..841b&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 86, Oct. 1974, p. 841, 842.

Other

36

Prisms, Refracting Telescopes, Schmidt Telescopes, Spectrum Analysis, Astronomical Spectroscopy, Magellanic Clouds, Seyfert Galaxies, Stellar Spectra

Scientific paper

An objective prism (diameter 61 cm) has been designed and built for low-dispersion spectral classification with a Schmidt telescope. The prism allows the recognition of certain natural spectral-type groups up to photographic magnitude 16.0, and should therefore be a valuable tool in spectral surveys of the Magellanic Clouds, and of other selected regions of the sky.

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