Giant Ringlike Radio Structures Around Galaxy Cluster Abell 3376

dc.contributor.authorBagchi, Joydeep
dc.contributor.authorDurret, Florence
dc.contributor.authorPaul, Surajit
dc.contributor.authoret al.
dc.date.accessioned2012-03-06T05:02:36Z
dc.date.available2012-03-06T05:02:36Z
dc.date.issued2007-11-09
dc.description.abstractIn the current paradigm of cold dark matter cosmology, large-scale structures are assembling through hierarchical clustering of matter. In this process, an important role is played by megaparsec (Mpc)-scale cosmic shock waves, arising in gravity-driven supersonic flows of intergalactic matter onto dark matter-dominated collapsing structures such as pancakes, filaments and clusters of galaxies. Here we report Very Large Array telescope observations of giant (∼ 2 Mpc ×1.6 Mpc), ring-shaped non-thermal radio emitting structures, found at the outskirts of the rich cluster of galaxies Abell 3376. These structures may trace the elusive shock waves of cosmological large scale matter flows, which are energetic enough to power them. These radio sources may also be the acceleration sites where magnetic shocks are possibly boosting 1cosmic-ray particles with energies of up to 1018 to 1019 electron volts.en_US
dc.identifier.urihttp://hdl.handle.net/11007/612
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprint;22/09
dc.subjectRadio Structuresen_US
dc.subjectCluster Abell 3376en_US
dc.titleGiant Ringlike Radio Structures Around Galaxy Cluster Abell 3376en_US
dc.typeArticleen_US

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