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Near-infrared imaging of ellipticals: surface brightness profiles and photometry.
- Source :
- Monthly Notices of the Royal Astronomical Society; 5/21/2003, Vol. 341 Issue 3, p747-759, 13p
- Publication Year :
- 2003
-
Abstract
- ABSTRACT We present near-infrared K-band imaging of a large sample of candidate merger remnant galaxies and Hickson Compact Group ellipticals. We derive light profile indices, effective radii and surface brightnesses, as well as total K-band magnitudes. We find that the light distributions of the merger remnant candidates are consistent with those of ‘normal’ ellipticals, and scatter around a mean profile index of (1/n) = 0.20 . Many of our sample galaxies have surface brightness profiles that are not well described by a de Vaucouleurs law (1/n= 0.25) , and we discuss the implications of this on the derived total magnitudes. Comparing the total K magnitudes calculated by extrapolating a de Vaucouleurs profile and those derived using a generalized Sérsic form, we find that a significant bias is introduced if the de Vaucouleurs law is not a good description of the actual light profile. [ABSTRACT FROM AUTHOR]
- Subjects :
- GALAXIES
ELLIPTICAL galaxies
ASTRONOMICAL photometry
Subjects
Details
- Language :
- English
- ISSN :
- 00358711
- Volume :
- 341
- Issue :
- 3
- Database :
- Complementary Index
- Journal :
- Monthly Notices of the Royal Astronomical Society
- Publication Type :
- Academic Journal
- Accession number :
- 9732712
- Full Text :
- https://doi.org/10.1046/j.1365-8711.2003.05947.x