Abstract
Abstract
Based on 16,283 early-type galaxies (ETGs) in 0.025 ≤ z
spec < 0.055 from Sloan Digital Sky Survey data, we show that the fundamental plane (FP) of ETGs is not a plane in the strict sense but is a curved surface with a twisted shape whose orthogonal direction to the surface is shifted as the central velocity dispersion (σ
0) or mean surface brightness within the half-light radius (μ
e
) changes. When ETGs are divided into subsamples according to σ
0, the coefficient of μ
e
of the FP increases, whereas the zero-point of the FP decreases at higher σ
0. Taking the z band as an example, the coefficient of μ
e
rises from 0.28 to 0.36 as σ
0 increases from ∼100 to ∼300 km s−1. At the same time, the zero-point of the FP falls from −7.5 to −9.0 in the same σ
0 range. The consistent picture on the curved nature of the FP is also reached by inspecting changes in the FP coefficients for ETG subsamples with different μ
e
. By examining scaling relations that are projections of the FP, we suggest that the warped nature of the FP may originate from dry merger effects that are imprinted more prominently in ETGs with higher masses.
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
2 articles.
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