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1
Multi-Wavelength Comparison of
3C273
This three-panel image shows the jet blasting out of the core of quasar 3c273. The scale on all three images is the same (about 10 arcseconds from one of the jet to the another.) This comparative display demonstrates the different intensities discovered in various regimes of the electromagnetic spectrum in this jet. From left to right, the images are optical (HST), X-ray (Chandra), and radio (MERLIN).
(Credit: Optical: NASA/STScI X-ray: NASA/CXC Radio: MERLIN)
This three-panel image shows the jet blasting out of the core of quasar 3c273. The scale on all three images is the same (about 10 arcseconds from one of the jet to the another.) This comparative display demonstrates the different intensities discovered in various regimes of the electromagnetic spectrum in this jet. From left to right, the images are optical (HST), X-ray (Chandra), and radio (MERLIN).
(Credit: Optical: NASA/STScI X-ray: NASA/CXC Radio: MERLIN)
2
Optical Image of 3C273
An optical image of the quasar 3C273 as observed by the Hubble Space Telescope..
(Credit: NASA/STScI)
An optical image of the quasar 3C273 as observed by the Hubble Space Telescope..
(Credit: NASA/STScI)
3
Radio Image of 3C273
This image of 3C273 was taken by the radio array of telescopes around Great Britain known as the Multi-Element Radio Linked Interferometer Network (MERLIN).
(Credit: MERLIN)
This image of 3C273 was taken by the radio array of telescopes around Great Britain known as the Multi-Element Radio Linked Interferometer Network (MERLIN).
(Credit: MERLIN)
4
Chandra X-ray Image with Scale
Bar
Scale bar = 5 arcsec
(Credit: NASA/CXC/SAO/H.Marshall et al.)
Scale bar = 5 arcsec
(Credit: NASA/CXC/SAO/H.Marshall et al.)
Return to Cycle 1 3C273 (06 Nov 00)