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Magnetar Rotating
Magnetars are rapidly spinning ultra-magnetic neutron stars with a period of between 3 and 12 seconds and are subject to "starquakes". As their phenomenal magnetic field shifts, the stellar crust breaks and emits bursts of gamma rays. These stars are all that remains of huge stars which have collapsed.
Magnetar Rotating2019-05-07T07:40:41ZMagnetars are rapidly spinning ultra-magnetic neutron stars with a period of between 3 and 12 seconds and are subject to "starquakes". As their phenomenal magnetic field shifts, the stellar crust breaks and emits bursts of gamma rays. These stars are a...PT21Shttps://d38zjy0x98992m.cloudfront.net/5000b36b-505a-4760-af1c-433af02863af/MAGNETAR_UHD_265_xlarge.jpghttps://d38zjy0x98992m.cloudfront.net/5000b36b-505a-4760-af1c-433af02863af/MAGNETAR_UHD_265_mp4_hd_video.mp4https://www.scientific.pictures/media/5000b36b-505a-4760-af1c-433af02863af/pricehttps://www.scientific.pictures/media/5000b36b-505a-4760-af1c-433af02863af/price
Supernova and Remnant SN1AX1970-01-01T00:00:00+00:00This animation shows a very dense white dwarf star devouring a much larger, but less massive, red star. The matter swirls into the white dwarf via an accretion disk. The white dwarf reaches a critical mass and undergoes a thermonuclear explosion that d...PT16Shttps://d38zjy0x98992m.cloudfront.net/dc3b4dd8-1df9-44bd-8b0b-65e4cd510c45/Supernova_and_Remnant_SN1AX_16sec_HQ_xlarge.jpghttps://d38zjy0x98992m.cloudfront.net/dc3b4dd8-1df9-44bd-8b0b-65e4cd510c45/Supernova_and_Remnant_SN1AX_16sec_HQ_mp4_hd_video.mp4https://www.scientific.pictures/media/dc3b4dd8-1df9-44bd-8b0b-65e4cd510c45/pricehttps://www.scientific.pictures/media/dc3b4dd8-1df9-44bd-8b0b-65e4cd510c45/price