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X9: A Special Kind of Neutron Star in the Globular Cluster 47 Tucanae #3567541 (License: Personal Use)
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The image visualizes X9, a unique low-mass X-ray binary located in the globular cluster 47 Tucanae, believed to consist of a neutron star and a white dwarf orbiting every 28 minutes-the shortest orbital period known for such a system. The inset shows real Chandra X-ray Observatory data pinpointing X9 (labeled) among cluster stars. The main artwork highlights relativistic effects, including Doppler-boosted emission and frame-dragging near the compact object.
Used in astronomy news articles, educational resources, and press releases about exotic stellar remnants; targets users searching for “neutron star X9”, “ultra-compact binary”, or “47 Tucanae discoveries”.
Related Cliparts: Discover X9, an unusual neutron star binary system in 47 Tucanae-possibly the first known ultra-compact X-ray binary with a white dwarf donor.
(view all X9: A Special Kind of Neutron Star in the Globular Cluster 47 Tucanae)
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