Arc statistics with realistic cluster potentials: I. method and first results
{}From the lensing properties of a numerically simulated cluster, from the statistical properties of the giant arcs produced by the cluster, and from comparing the cluster properties derived both from lensing and from the X-ray properties of the intracluster gas, we conclude (1) that clusters may be...
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| Autori principali: | , |
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| Natura: | Article (Journal) Chapter/Article |
| Lingua: | inglese |
| Pubblicazione: |
30 November 1993
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| In: |
Arxiv
Year: 1993, Pages: 1-26 |
| DOI: | 10.48550/arXiv.astro-ph/9311074 |
| Accesso online: | Resolving-System, kostenfrei, Volltext: https://doi.org/10.48550/arXiv.astro-ph/9311074 Verlag, kostenfrei, Volltext: http://arxiv.org/abs/astro-ph/9311074 
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| Note sull'autore: | Matthias Bartelmann und Achim Weiss |
| Riassunto: | {}From the lensing properties of a numerically simulated cluster, from the statistical properties of the giant arcs produced by the cluster, and from comparing the cluster properties derived both from lensing and from the X-ray properties of the intracluster gas, we conclude (1) that clusters may be significantly more efficient for lensing than estimated from their velocity dispersion on the basis of iso- thermal-sphere models, (2) that the discrepancy between cluster core radii derived from lensing and from their X-ray surface brightness may be understood assuming that the intracluster gas was expelled from the cluster galaxies when the dark `body' of the cluster had already formed, and (3) that clusters may be efficient in producing giant arcs even if they have extended cores and a fairly shallow sur- face-density profile. This may mean that arcs may be much easier to produce, and therefore more abundant, than previously estimated. |
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| Descrizione del documento: | Gesehen am 29.09.2017 |
| Descrizione fisica: | Online Resource |
| DOI: | 10.48550/arXiv.astro-ph/9311074 |