New HST and Chandra results on the jet in 3C273

Details New HST and Chandra results on the jet in 3C273 New HST and Chandra results on the jet in 3C273

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...206.3014j&link_type=abstract

American Astronomical Society Meeting 206, #30.14; Bulletin of the American Astronomical Society, Vol. 37, p.475

Astronomy and Astrophysics

Astronomy

Scientific paper

We will present results from two recent imaging campaigns on the jet of 3C273. We have obtained UV data at 180nm with ACS/SBC, which probe the possible connection between the jet's UV and X-ray emission. Chandra was used to monitor 3C273's jet over Cycle 5 to detect possible variability that would indicate synchrotron emission, at the same time tripling the number of detected X-ray photons, which allows for more precise determination of the X-ray spectral evolution along the jet.
Work at Fermilab was supported by the US Department of Energy under contract No. DE-AC02-76CH03000, and by NASA contract NAS8-03060. Work at MIT was supported under SAO contract SV3-73016 for the Chandra X-ray Center, operated by SAO under NASA contract NAS8-03060. Work at SAO was supported by NASA contract NAS8-03060.

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