Giant luminous arc statistics and mass distribution of cluster of galaxies.

Details Giant luminous arc statistics and mass distribution of cluster of galaxies. Giant luminous arc statistics and mass distribution of cluster of galaxies.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..585h&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 585 - 586

Astronomy and Astrophysics

Astrophysics

Clusters Of Galaxies: Luminous Arcs, Clusters Of Galaxies: Mass Distribution

Scientific paper

The authors have constructed an arc identification scheme by fully taking into account both the detection conditions in the arc survey and the evolution of the source galaxies. The scheme has been applied to Le Fèvre et al.'s (1994) arc survey data in order to constrain the models of cluster mass distribution. The authors have found that any presently assumed spherical cluster mass distribution models even with very small core radius cannot reproduce the large number observed in Le Fèvre et al.'s arc survey.

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