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- W2100056077 abstract "Abstract We use density and temperature profiles obtained from XMM‐Newton observations to derive a potential of NGC 5846 out to 11 R e , thus probing the mass distribution deep into the halo. The inferred circular velocity is significantly higher than the extrapolation of dynamical models implying a halo, more massive than previously thought. Using an I ‐band surfacebrightness profile and a projected velocity dispersion profile consisting of long‐slit kinematic measurements and planetary nebulae (PNe) velocity dispersions, we solve the Jeans equations, assuming a non‐rotating spherical system. The solutions suggest a highly radially anisotropic galaxy outside 0.7 R e with β ∼ 0.75. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)" @default.
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- W2100056077 date "2008-11-25" @default.
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- W2100056077 title "The orbital structure of the massive elliptical galaxy NGC 5846" @default.
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- W2100056077 doi "https://doi.org/10.1002/asna.200811052" @default.
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