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The discovery of ASKAP J1935+2148, a long-period radio transient with a period of 53.8 minutes, reveals three distinct emission states: a bright pulse state, a weak pulse state, and a quiescent state. This source challenges current astrophysical models, particularly regarding neutron stars, as it exhibits significant variations in emission modes and properties. The findings suggest that ASKAP J1935+2148 may represent a new class of astrophysical objects, bridging the gap between known long-period sources.
- Author
- Max Stewart
- Language
- EN