Distribution of surface brightness in Seyfert galaxies. I - Sample. Results of scanning

Details Distribution of surface brightness in Seyfert galaxies. I - Sample. Results of scanning Distribution of surface brightness in Seyfert galaxies. I - Sample. Results of scanning

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986afz....24..333a&link_type=abstract

(Astrofizika, vol. 24, Mar.-Apr. 1986, p. 333-348) Astrophysics (ISSN 0571-7132), vol. 24, no. 2, Sept. 1986, p. 194-203. Transl

Astronomy and Astrophysics

Astrophysics

6

Astronomical Photometry, Brightness Distribution, Seyfert Galaxies, Spiral Galaxies, Galactic Structure, Scanning

Scientific paper

A sample of 45 spiral galaxies including 19 Seyfert objects is formed within distances less than 100 Mpc (H0 = 75 km s-1Mpc-1). Small aperture measurements in B with a scanning photoelectric photometer were made to obtain the surface brightness distributions along the major axes in 14 galaxies. The characteristic parameters such as the surface brightness and its gradient at the distance of 1 kpc from the center of galaxies are calculated.

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