Galaxies with strong narrow emission lines - Spectroscopy, morphology and range in absolute sizes

Details Galaxies with strong narrow emission lines - Spectroscopy, morphology and range in absolute sizes Galaxies with strong narrow emission lines - Spectroscopy, morphology and range in absolute sizes

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.191..391f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 191, May 1980, p. 391-397.

Mathematics

Logic

16

Astronomical Spectroscopy, Emission Spectra, Galactic Radiation, H Beta Line, Galactic Nuclei, H Ii Regions, Line Spectra, Morphology

Scientific paper

A sample of 47 Tololo emission line galaxies and new spectroscopy for 29 of these galaxies are presented. The galaxies are classified morphologically into: (1) entire galaxy is emission line source, (2) outer regions are emission line source which appear to be normal or supersized H II regions in late type galaxies, (3) nucleus only is emission line source, and (4) multiple systems with a high H beta/4959 ratio.

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