An objective prism H-alpha survey of nearby clusters of galaxies. I - Abell 347 and Abell 1367

Astronomy and Astrophysics – Astronomy

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Galactic Clusters, Galactic Radiation, H Alpha Line, Astronomical Photometry, Forbidden Bands, Spectral Line Width, Spectrophotometry

Scientific paper

The Burrell Schmidt telescope has been used to survey H-alpha emission in 69 galaxies in the Abel 347 and Abell 1367 clusters. The survey has recovered 60-80 percent of the potentially detectable IRAS galaxies. An approximate flux threshold of about 10 to the -13th erg/sq cm per s and an equivalent width threshold of about 20 A have been found. Global H-alpha + forbidden N II line equivalent widths and fluxes were found to be in good agreement with values obtained for a small subset of galaxies measured using wide aperture photoelectric photometry. It is noted that an approximate redshift estimate may be made with 1sigma accuracy of about 550 km/s by measuring the position of the H-alpha emission feature relative to the peak of the continuum spectrum.

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