Kinematics and morphological type of the Seyfert galaxy NGC 4507

Details Kinematics and morphological type of the Seyfert galaxy NGC 4507 Kinematics and morphological type of the Seyfert galaxy NGC 4507

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aj.....89.1514a&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 89, Oct. 1984, p. 1514-1519.

Mathematics

Logic

8

Astronomical Spectroscopy, Galactic Structure, High Dispersion Spectrographs, Kinematics, Seyfert Galaxies, Classifications, Disk Galaxies, Galactic Nuclei, Galactic Rotation, Line Spectra, Oxygen Spectra

Scientific paper

Long-slit, medium-high dispersion optical spectroscopy and direct imaging of the class 2 Seyfert galaxy NGC 4507 are reported. The results are consistent with the morphological classification SBab(rs)I given in the Revised Shapley-Ames Catalog. Evidence has been found that the nuclear forbidden O III line emitting region is structurally and kinematically distinct from the galaxy disk. The distribution of line profiles over this nuclear region is presented and its kinematics discussed.

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