The giant luminous arc Statistics. II. spherical lens models based on ROSAT HRI data

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dc.creatorMolikawa, Kohji
dc.creatorHattori, Makoto
dc.creatorKneib, Jean-Paul
dc.creatorYamashita, Kazuyuki
dc.date1999-09-10
dc.date.accessioned2026-07-07T02:33:12Z
dc.date.available2026-07-07T02:33:12Z
dc.descriptionWe present ROSAT HRI X-ray observations of all the galaxy clusters in the Le Fèvre et al. arc survey sample in order to study the spatial distribution of the intra-cluster medium, and examine the expected number of giant luminous arcs for the sample using two spherically symmetric lens models constrained by our X-ray data.
dc.description16 pages including 1 figure. Figures in the appendix are not included. Accepted for publication in Astronomy and Astrophysics, Main Journal
dc.identifierhttps://arxiv.org/abs/astro-ph/9909180
dc.identifierhttp://arxiv.org/abs/astro-ph/9909180
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14749
dc.subjectAstrophysics
dc.titleThe giant luminous arc Statistics. II. spherical lens models based on ROSAT HRI data
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