Objective prism survey of emission-line galaxies. IV

Details Objective prism survey of emission-line galaxies. IV Objective prism survey of emission-line galaxies. IV

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991acaps..11...28h&link_type=abstract

(Acta Astrophysica Sinica, vol. 11. no. 1, 1991, p. 28-37) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 15, June 19

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Emission Spectra, Galaxies, Sky Surveys (Astronomy), Astronomical Catalogs, Dwarf Galaxies, Line Spectra, Seyfert Galaxies, Spiral Galaxies, Ultraviolet Spectra

Scientific paper

The results of an objective prism survey of emission-line galaxies using the Beijing Observatory 60-cm Schmidt are given. The survey includes 100 emission-line objects, of which 96 are emission-line galaxies, 3 are planetary nebulae and 1 is an emission-line star. Of the emission-line galaxies, 69-72 percent are of types s or sd; 27-28 percent are of types d and ds. In addition to 4 known Seyfert galaxies, there are at least 5 probable Seyferts. Twenty-three of the objects are IRAS sources characterized by strong emission phenomena.

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