Kes 75 vs SN 1006
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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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SN 1006
SN 1006 is a supernova remnant located within the Lupus nebula of our Milky Way galaxy. It represents the expanding debris field from a Type Ia supernova event that occurred around 1006 CE. This was the most luminous stellar explosion ever observed and remains notable for its brightness, detectable even during daylight hours. Astronomers study SN 1006 to understand supernovae, stellar evolution, a...
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