Multi-wavelength Look at 3C58
QuickTime MPEG This sequence compares Chandra's X-ray image of 3C58 with the views seen by optical and radio telescopes. The intricate X-ray loops in the Chandra image and the features in the radio images of 3C58 extend a dozen light years from the pulsar, likely representing the complex magnetic field structure there.
[Run Time: 0:32]
(Credit: X-ray: NASA/CXC/SAO/P.Slane et al.; Optical: DSS; Radio: NCSU/S.Reynolds)
QuickTime MPEG This sequence compares Chandra's X-ray image of 3C58 with the views seen by optical and radio telescopes. The intricate X-ray loops in the Chandra image and the features in the radio images of 3C58 extend a dozen light years from the pulsar, likely representing the complex magnetic field structure there.
[Run Time: 0:32]
(Credit: X-ray: NASA/CXC/SAO/P.Slane et al.; Optical: DSS; Radio: NCSU/S.Reynolds)
Comparison of 3C58 and the Crab Nebula
QuickTime MPEG In this series of X-ray images, the strong similarities between the center of 3C58 and the Crab Nebula pulsar -- one of the most famous objects in astronomy -- are shown. The 3C58 pulsar, the Crab Nebula pulsar, and a growing list of other pulsars offer dramatic proof that strong electromagnetic fields around rapidly rotating neutron stars are powerful generators of both high-energy particles and magnetic fields.
[Run Time: 0:22]
(Credit: 3C58: NASA/CXC/SAO/P.Slane et al.; Crab: NASA/CXC/ASU/J.Hester et al.)
QuickTime MPEG In this series of X-ray images, the strong similarities between the center of 3C58 and the Crab Nebula pulsar -- one of the most famous objects in astronomy -- are shown. The 3C58 pulsar, the Crab Nebula pulsar, and a growing list of other pulsars offer dramatic proof that strong electromagnetic fields around rapidly rotating neutron stars are powerful generators of both high-energy particles and magnetic fields.
[Run Time: 0:22]
(Credit: 3C58: NASA/CXC/SAO/P.Slane et al.; Crab: NASA/CXC/ASU/J.Hester et al.)
Layers of Chandra's 3-Color Image
QuickTime MPEG In this sequence, the individual layers that comprise the Chandra 3-color image of 3C58 are shown. The red layer represents the lower-energy X-rays, green shows the medium-energy range, and blue reveals the highest-energy X-rays observed by Chandra.
[Run Time: 0:20]
(Credit: NASA/CXC/SAO/P.Slane et al.)
QuickTime MPEG In this sequence, the individual layers that comprise the Chandra 3-color image of 3C58 are shown. The red layer represents the lower-energy X-rays, green shows the medium-energy range, and blue reveals the highest-energy X-rays observed by Chandra.
[Run Time: 0:20]
(Credit: NASA/CXC/SAO/P.Slane et al.)
Return to 3C58 (14 Dec 04)
Revised: July 28, 2008