Kes 75 vs E0102
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Kes 75
Kes 75 is a supernova remnant in the Milky Way, located in the direction of the constellation Aquila. Its interior contains PSR J1846-0258, a young, energetic neutron star classified as a high-magnetic-field pulsar and observed to produce magnetar-like bursts. The remnant and pulsar are studied together in X-rays because they provide evidence about particle acceleration, neutron-star activity, and...
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E0102
E0102, formally designated 1E 0102.2-7219, is a young, oxygen-rich supernova remnant located in the Small Magellanic Cloud, a dwarf galaxy orbiting the Milky Way. Estimated to be approximately 2,000 years old, it is the brightest X-ray source in its host galaxy and has been extensively studied by instruments like the Chandra X-ray Observatory. The remnant features a distinct, expanding ring of eje...
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