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                        RX J1856 in Optical Light
                        
This optical image of RX J1856.5-3754 portrays a crowded region of star formation. In comparison, the Chandra X-ray image shows that RX J1856 outshines all of the other sources in the field, indicating it is both extremely hot and very small.
(Credit: European Southern Observatory Very Large Telescope)
                 This optical image of RX J1856.5-3754 portrays a crowded region of star formation. In comparison, the Chandra X-ray image shows that RX J1856 outshines all of the other sources in the field, indicating it is both extremely hot and very small.
(Credit: European Southern Observatory Very Large Telescope)
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                        Size Comparison of RX J1856 to
                        Neutron and Quark Stars 
This artist's rendition shows the diameter of RX J1856.5-3754, determined by data from NASA's Chandra X-ray Observatory, is too small to be a neutron star. The data are consistent with predicted size for a strange quark star, an object never before seen in nature.
(Illustration: CXC/M. Weiss)
                 This artist's rendition shows the diameter of RX J1856.5-3754, determined by data from NASA's Chandra X-ray Observatory, is too small to be a neutron star. The data are consistent with predicted size for a strange quark star, an object never before seen in nature.
(Illustration: CXC/M. Weiss)
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                        Chandra X-ray Image of 3C58
                        
Chandra observations of 3C58, the remnants of a supernova noted on Earth in AD 1181, reveal that the neutron star in the core has a temperature much lower than expected. This suggests that a new state of nuclear matter might exist inside the star.
(Credit: NASA/CXC/CfA/P.Slane et al.)
                 Chandra observations of 3C58, the remnants of a supernova noted on Earth in AD 1181, reveal that the neutron star in the core has a temperature much lower than expected. This suggests that a new state of nuclear matter might exist inside the star.
(Credit: NASA/CXC/CfA/P.Slane et al.)
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                 Return to RX J1856.5-3754 and 3C58 (10 Apr 02)







