Giant Ringlike Radio Structures Around Galaxy Cluster Abell 3376

Author:

Bagchi Joydeep1234,Durret Florence1234,Neto Gastão B. Lima1234,Paul Surajit1234

Affiliation:

1. The Inter-University Centre for Astronomy and Astrophysics (IUCAA), Post Bag 4, Ganeshkhind, Pune University Campus, Pune 411007, India.

2. Institut d'Astrophysique de Paris, UMR-7095, CNRS, Université Pierre et Marie Curie, Paris, France, and Observatoire de Paris-Meudon, LERMA, Paris, France.

3. Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, São Paulo, Brazil 05508-900.

4. Institut fur Theoretische Physik und Astrophysik, Universität Würzburg, Sanderring 2, 97070 Würzburg, Germany.

Abstract

In 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 by 1.6 Mpc), ring-shaped nonthermal 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 cosmic-ray particles with energies of up to 10 18 to 10 19 electron volts.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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