Distribution of surface brightness in Seyfert galaxies. II - Multiaperture photometry

Details Distribution of surface brightness in Seyfert galaxies. II - Multiaperture photometry Distribution of surface brightness in Seyfert galaxies. II - Multiaperture photometry

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986afz....24..425a&link_type=abstract

(Astrofizika, vol. 24, May-June 1986, p. 425-435) Astrophysics (ISSN 0571-7132), vol. 24, no. 3, Nov. 1986, p. 241-248. Translat

Astronomy and Astrophysics

Astrophysics

2

Astronomical Spectroscopy, Brightness Distribution, Electrophotometry, Seyfert Galaxies, Surface Properties, Apertures, Galactic Nuclei

Scientific paper

Photoelectric surface brightness distributions are calculated using multiaperture photometry in B in 10 normal and Seyfert galaxies of the sample discussed in the first paper. A comparison of surface brightness profiles from photoelectric scans along the major axis with those of multiaperture photometry shows that the latter are accurate within about 0m.2/sq. arc sec for galaxies with low or moderate inclination. No statistical significant differences were found between the color indexes of the central regions of normal and Seyfert galaxies.

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