2015/08/21 by Madoka Itahana, Motokazu Takizawa, Hiroki Akamatsu +5 · 3 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics and Cosmic Phenomena #Galaxies: Formation, Evolution, Phenomena #Galaxy cluster #Intracluster medium #Mach number #Magnetic field #Particle acceleration #Radio galaxy #Shock (circulatory) #Spectral index #Surface brightness #astro-ph.CO #astro-ph.HE
paper · pdf · doi:10.1093/pasj/psv084
12 pages, 11 figures, accepted for publication in PASJ
arxiv created 2015/08/21 · openalex publication_date 2015/10/06 · arxiv updated 2015/10/14 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Abstract We present the results of Suzaku observations of the galaxy cluster 1RXS J0603.3+4214 with the “Toothbrush” radio relic. Although a shock with Mach number M ≃ 4 is expected at the outer edge of the relic from the radio observation, our temperature measurements of the intracluster medium indicate a weaker temperature difference than expected. The Mach number estimated from the temperature difference at the outer edge of the relic is M ≃ 1.5, which is significantly lower than the value estimated from the radio data even considering both statistical and systematic errors. This suggests that a diffusive shock acceleration theory in the linear test particle regime, which is commonly used to link the radio spectral index to the Mach number, is invalid for this relic. We also measured the temperature difference across the western part of the relic, where a shock with M ≃ 1.6 is suggested from the X-ray surface brightness analysis of the XMM-Newton data, and obtained consistent results in an independent way. We searched for the non-thermal inverse Compton component in the relic region and the resultant upper limit on the flux is 2.4 × 10−13 erg cm−2 s−1 in the 0.3–10 keV band. The lower limit of the magnetic field strength becomes 1.6 μG, which means that magnetic energy density could be more than a few percent of the thermal energy.