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- W2136219126 endingPage "460" @default.
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- W2136219126 abstract "We report on the discovery of a rapidly corotating stellar and gas component in the nucleus of the shell elliptical NGC 2865. The stellar component extends ~ 0.51 h100−1 kpc along the major axis, and shows depressed velocity dispersion and absorption-line profiles skewed in the opposite sense to the mean velocity. Associated with it is a young stellar population with enhanced Hβ, lowered Mg, and the same Fe indices relative to the underlying elliptical. Its recent star formation history is constrained by considering ‘bulge+burst’ models under four physically motivated scenarios, using evolutionary population synthesis. Scenarios in which the nuclear component is formed over a Hubble time or recently from continuous gas inflow are ruled out." @default.
- W2136219126 created "2016-06-24" @default.
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- W2136219126 date "1999-06-21" @default.
- W2136219126 modified "2023-09-25" @default.
- W2136219126 title "The shell elliptical galaxy NGC 2865: evolutionary population synthesis of a kinematically distinct core" @default.
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- W2136219126 doi "https://doi.org/10.1046/j.1365-8711.1999.02526.x" @default.
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