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Galaxy merging and the Fundamental Plane of elliptical galaxies

We present preliminary results of numerical simulations of dissipationless merging of stellar systems, aimed at exploring the consequences of merging between gas free, spheroidal systems. In particular, we study the dynamical and structural characteristics of hierarchical merging between equal mass stellar systems, and we compare the properties of the end-products with the most important structural and dynamical scaling relations obeyed by spheroids. In the explored hierarchy of four successive mergings we find that the FP tilt is marginally conserved, but both the Faber-Jackson and Kormendy relations are not conserved.

preprint2001arXivOpen access
Carlo NipotiPasquale LondrilloLuca Ciotti
astro-ph
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Open access3 authors1 topic
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Carlo NipotiPasquale LondrilloLuca Ciotti

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