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Cropped millisecond pulsar

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Animation showing neutron star and accretion disk evolving into a millisecond pulsar, with magnetic fields. The formation of a pulsar: A star in a binary star system has collapsed to a neutron star. It begins to gain material from its companion star (known as "accretion"). The infalling matter causes it to speed up and begin emitting high energy radiation, eventually forming a pulsar rotating at up to 1000 times a second. This is a shortened version of the original video with the last 10 seconds removed. This is because the end of the video contains rapid flashing lights that may be triggering to photosensitive viewers.

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1:02

NASA-JAXA XRISM Mission Sees Pulsar Accreting Companion's 'Wind' (SVS15099)

NASA's Scientific Visualization Studio - NASA’s Goddard Space Flight Center Conceptual Image LaboratoryAlt text: Animation of the BP Crucis system0:00 A wide view, showing the giant star, its gas stream, and the pulsar nearing it. 0:08 The camera zooms into the pulsar as it encounters the stream. 0:10 Gas flowing past the pulsar forms a clockwise-spinning accretion disk. 0:17 The disk breaks up. The gas now flows directly onto the pulsar. 0:35 As the pulsar nears the end of its passage through the stream, a new disk, spinning counterclockwise, forms. 0:51 The disk breaks up and the pulsar exits the stream. 0:52 Return to a wide view of the system.
0:20

Swift Spacecraft Animations- 2025 (SVS14786 - SWIFT 360 4k 60fps, cropped)

NASA's Scientific Visualization Studio - eMITS/Adriana Manrique Gutierrez, eMITS/Jonathan North, eMITS/Michael Lentz, eMITS/Scott Wiessinger, eMITS/Sophia Roberts, University of Maryland College Park/Francis Reddy, University of Maryland College Park/Jeanette Kazmierczak, NASA/GSFC/Brad Cenko, NASA/GSFC/Regina Caputo