Preliminary results of the Baranne white pupil image tube nebular spectrograph

Details Preliminary results of the Baranne white pupil image tube nebular spectrograph Preliminary results of the Baranne white pupil image tube nebular spectrograph

Jul 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974rpnl.conf..231b&link_type=abstract

In European Southern Obs. Res. Programmes for the New Large Telescopes p 231-237 (SEE N75-15523 06-89)

Computer Science

Performance

5

Emission Spectra, Image Tubes, Spectroscopic Telescopes, Astronomical Spectroscopy, Galaxies, H Ii Regions, H Lines, Nebulae, Visual Observation

Scientific paper

The Baranne white pupil spectrograph optical characteristics are described. The spectrograph allows a direct picture of the astronomical object at the same time as the spectrum. This accurate check of the slit position plays an important role in the study of any fine features in the H II region of galaxies. A spectrum of the galaxies M 82 and NGC 3079 are given as an example of its performance.

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