CCD photometry of Seyfert galaxies

Details CCD photometry of Seyfert galaxies CCD photometry of Seyfert galaxies

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.157..145m&link_type=abstract

(Instituto de Astrofisica de Canarias and Comision Interministerial de Ciencia y Tecnologia, Summer School on Evolutionary Pheno

Astronomy and Astrophysics

Astrophysics

9

Astronomical Photometry, Charge Coupled Devices, Seyfert Galaxies, Elliptical Galaxies, Infrared Photometry, Spiral Galaxies, Visual Photometry

Scientific paper

Morphology and elliptically averaged luminosity profiles have been derived from CCD surface photometry of thirteen Seyfert galaxies. Apparent V and I magnitudes, V - I color index, as well as absolute Mv and MI magnitudes have been calculated. V and I luminosity profiles of Mk 10, Mk 79, Mk 358, Mk 618, Mk 352, and Mk 110, are adjusted by the usual model bulge plus disk with structural parameters comparable to those observed in normal spirals. The averaged luminosity profiles of Mk 50, Mk 124, Mk 348, and 3C227 are fitted by r exp -1/4 law with structural parameters similar to those observed in ellipticals and red compact galaxies. Mk 42 and NGC 985 show disturbed luminosity profiles.

Affiliated with

Also associated with

No associations

Rating

CCD photometry of Seyfert galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with CCD photometry of Seyfert galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CCD photometry of Seyfert galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1703519