Radio and X-ray Observations of 3C303 and 3C15

Details Radio and X-ray Observations of 3C303 and 3C15 Radio and X-ray Observations of 3C303 and 3C15

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xrrc.proce7.13e&link_type=abstract

"X-Ray and Radio Connections (eds. L.O. Sjouwerman and K.K Dyer) Published electronically by NRAO, http://www.aoc.nrao.edu/event

Computer Science

X-Ray, Radio, Dissipation Of Jets

Scientific paper

We describe the Chandra detection of X-ray kpc-scale jet components in 3C303 and 3C15. The X-ray morphology of 3C303 is similar to that of the radio/optical emission with peaks in the X-ray emission found at 5.5 arcsec, 9 arcsec and 17 arcsec from the core. In 3C15, the peak of the X-ray emission in the jet is 4.1 arcsec from the core, and coincident with a component previously identified in the radio and optical jets. We construct the spectral energy distributions for components in these sources and find that the X-ray fluxes are well below the extrapolation of the radio-to-optical continuum. We provide interpretations of these observations, and describe planned very long baseline interferometry observations to study the parsec scale jet morphology.

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