Chandra detection of hotspot and knots of 3C 303

Jun Kataoka, P. Edwards, M. Georganopoulos, F. Takahara, S. Wagner

Research output: Contribution to journalArticle

34 Citations (Scopus)

Abstract

We report the detection at X-rays of the radio/optical hotspot and knots of 3C 303 from a short (15 ksec) Chandra exposure in 2001 March. The X-ray morphology is similar to that of the radio/optical emission with peaks in the X-ray emission found at 5.5 inches (knot B), 9 inches (knot C) and 17 inches (hotspot) from the core of 3C 303. Despite the limited signal-to-noise ratio of the short Chandra exposure, the X-ray photon spectrum was measured for the hotspot. We construct the spectral energy distribution (SED) and find that the X-ray flux is well below the extrapolation of the radio-to-optical continuum, which we interpret as resulting from the production of X-rays via inverse Compton scattering of both synchrotron photons (SSC) and cosmic microwave background photons (EC/CMB). The magnetic field strength, region size, and the maximum energy of electrons are self-consistently determined for the hotspot to be B ≃ 4.3 μG, R ≃ 6.5 × 1021 cm, and γmax ≃ 1.4 × 107. This implies a magnetic field strength a factor of ∼30 below the equipartition value; Beq ≃ 150 μG. The origin of this large departure from equipartition is still uncertain, but the discrepancy is reduced if the plasma in the hotspot is moving with mildly relativistic speeds. Our observation of 3C 303, as well as recent Chandra detections of large scale jets and hotspots in a number of radio galaxies, confirm that particles are accelerated very efficiently in radio galaxies.

Original languageEnglish
Pages (from-to)91-97
Number of pages7
JournalAstronomy and Astrophysics
Volume399
Issue number1
Publication statusPublished - 2003 Feb
Externally publishedYes

Fingerprint

radio
x rays
radio galaxies
field strength
photons
magnetic field
radio emission
spectral energy distribution
magnetic fields
signal-to-noise ratio
light emission
energy
detection
extrapolation
synchrotrons
signal to noise ratios
scattering
continuums
plasma
microwaves

Keywords

  • Galaxies: active
  • Galaxies: individual: 3C 303
  • Galaxies: jets
  • X-rays: galaxies

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Kataoka, J., Edwards, P., Georganopoulos, M., Takahara, F., & Wagner, S. (2003). Chandra detection of hotspot and knots of 3C 303. Astronomy and Astrophysics, 399(1), 91-97.

Chandra detection of hotspot and knots of 3C 303. / Kataoka, Jun; Edwards, P.; Georganopoulos, M.; Takahara, F.; Wagner, S.

In: Astronomy and Astrophysics, Vol. 399, No. 1, 02.2003, p. 91-97.

Research output: Contribution to journalArticle

Kataoka, J, Edwards, P, Georganopoulos, M, Takahara, F & Wagner, S 2003, 'Chandra detection of hotspot and knots of 3C 303', Astronomy and Astrophysics, vol. 399, no. 1, pp. 91-97.
Kataoka J, Edwards P, Georganopoulos M, Takahara F, Wagner S. Chandra detection of hotspot and knots of 3C 303. Astronomy and Astrophysics. 2003 Feb;399(1):91-97.
Kataoka, Jun ; Edwards, P. ; Georganopoulos, M. ; Takahara, F. ; Wagner, S. / Chandra detection of hotspot and knots of 3C 303. In: Astronomy and Astrophysics. 2003 ; Vol. 399, No. 1. pp. 91-97.
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