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A deep Chandra observation of the Perseus cluster: shocks and ripples

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Fabian, A. C., Sanders, J. S., Allen, S. W., Crawford, C. S., Iwasawa, K., Johnstone, R. M., Schmidt, R. W., Taylor, G. B.·2003·Monthly Notices of the Royal Astronomical Society

Abstract

We present preliminary results from a deep observation lasting almost 200 ks of the centre of the Perseus cluster of galaxies around NGC 1275. The X-ray surface brightness of the intracluster gas beyond the inner 20 kpc, which contains the inner radio bubbles, is very smooth apart from some low-amplitude quasi-periodic ripples. A clear density jump at a radius of 24 kpc to the north-east, about 10 kpc out from the bubble rim, appears to be due to a weak shock driven by the northern radio bubble. A similar front may exist around both inner bubbles but is masked elsewhere by rim emission from bright cooler gas. The continuous blowing of bubbles by the central radio source, leading to the propagation of weak shocks and viscously dissipating sound waves seen as the observed fronts and ripples, gives a rate of working which balances the radiative cooling within the inner 50 kpc of the cluster core.

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Metadata

Authors
Fabian, A. C., Sanders, J. S., Allen, S. W., Crawford, C. S., Iwasawa, K., Johnstone, R. M., Schmidt, R. W., & Taylor, G. B.
Venue
Monthly Notices of the Royal Astronomical Society
Published
2003-09
Volume
344
Issue
3
Pages
L43-L47
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2099782510
Cited by
619
References
0
FWCI
30.54
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: A deep Chandra observation of the Perseus cluster: shocks and ripples. https://app.cochat.ai/papers/10.1046/j.1365-8711.2003.06902.x
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Fabian, A. C., Sanders, J. S., Allen, S. W., Crawford, C. S., Iwasawa, K., Johnstone, R. M., Schmidt, R. W., & Taylor, G. B. (2003). A deep Chandra observation of the Perseus cluster: shocks and ripples. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1046/j.1365-8711.2003.06902.x

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