Skip to main content
Log in

Discovery of a Giant Radio Halo in a Massive Merging Cluster at z = 0.443

  • Published:
Journal of Astrophysics and Astronomy Aims and scope Submit manuscript

Abstract

We have discovered a giant radio halo in the massive merging cluster MACSJ0417.5-1154. This cluster, at a redshift of 0.443, is one of the most X-ray luminous galaxy cluster in the MAssive Cluster Survey (MACS) with an X-ray luminosity in the 0.1–2.4 keV band of 2.9×1045 erg s − 1. Recent observations from GMRT at 230 and 610 MHz have revealed a radio halo of ∼ 1.2 × 0.3 Mpc2 in extent. This halo is elongated along the North-West, similar to the morphology of the X-ray emission from Chandra. The 1400 MHz radio luminosity (L r) of the halo is ∼2 × 1025 W Hz − 1, in good agreement with the value expected from the L x − L r correlation for cluster halos.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Brunetti, G., Cassano, R., Dolag, K., Setti, G. 2009, Astron. Astrophys., 507, 661.

    Article  ADS  Google Scholar 

  • Ebeling, H., Edge, A. C., Mantz, A., Barrett, E., Henry, J. Patrick, Ma, C. J., van Speybroeck, L. 2010, Mon. Not. R. Astron. Soc., 407, 83.

    Article  ADS  Google Scholar 

  • Venturi, T., Giacintucci, S., Dallacasa, D., Cassano, R., Brunetti, G., Bardelli, S., Setti, G. 2008, Astron. Astrophys., 484, 327.

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to K. S. Dwarakanath.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Dwarakanath, K.S., Malu, S. & Kale, R. Discovery of a Giant Radio Halo in a Massive Merging Cluster at z = 0.443. J Astrophys Astron 32, 529–532 (2011). https://doi.org/10.1007/s12036-011-9109-1

Download citation

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s12036-011-9109-1

Keywords

Navigation