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- W2154795627 abstract "Studies of the proper motion of many filaments in the Crab Nebula show that the expansion centre does not coincide with the present position of the pulsar NP 0532. Possible reasons for this difference are discussed. Estimates of the turbulent velocity within the nebula indicate that it lies in the range 100 to 300 km sec−1. An analysis of the present expansion rate of the nebula indicates a convergence at 1140 ± 10 AD. The acceleration implied in this result could arise from magnetic or relativistic electron pressure." @default.
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- W2154795627 date "1971-01-01" @default.
- W2154795627 modified "2023-09-23" @default.
- W2154795627 title "Dynamics of the Crab Nebula" @default.
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- W2154795627 doi "https://doi.org/10.1007/978-94-010-3087-8_2" @default.
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