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- W3100660669 abstract "Abstract We present H -band observations of the elliptical galaxy NGC 4696, the brightest member of the Centaurus cluster of galaxies. We have measured its light profile, using a two-dimensional fitting algorithm, out to a radius of 180 arcsec (37 h 70 −1 kpc). The profile is well described by a de Vaucouleurs law, with an effective radius of 35.3 ± 1.0 h 70 −1 kpc. There is no need for the extra free parameter allowed by a Sérsic law. Allowing for a variation of 0.3% in the sky level, the profile obtained is compatible with data from the Two-Micron All Sky Survey (2MASS). The profile shows no sign of either a truncation or an extended halo." @default.
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- W3100660669 date "2006-01-01" @default.
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- W3100660669 title "The Near-Infrared Surface Brightness Distribution of NGC 4696" @default.
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- W3100660669 doi "https://doi.org/10.1071/as05037" @default.
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