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Results of observations next up previous
Next: The main observational parameters Up: Spectral survey of Case Previous: CCD observations and data

Results of observations

In this section we present the results of the spectra processing. We divided the presentation of the observed galaxies into the two main groups. In Tables 2 and 3 we give some general parameters, line intensities and equivalent widths for 142 galaxies with the detected emission lines. We summarize data in Table 4 for the rest 44 galaxies where we have not detected emission lines (in the blue part of the spectrum). One Case object CG 273 appeared to be a distant QSO. Its parameters are described separately after the main data. We present in Fig. 1 the spectra of seven emission-line galaxies and that of the quasar CG 273, in order to illustrate the main activity types in our sample.



 

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