The Discovery of a 41 s Radio Pulsar PSR J0311+1402 with ASKAP

The Discovery of a 41 s Radio Pulsar PSR J0311+1402 with ASKAP

The emerging population of long-period radio transients (LPTs) shows both similarities and differences with normal pulsars. A key difference is that their radio emission is too bright to be powered solely by rotational energy. Various models have been proposed (including both white dwarf or neutron...

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Bibliographic Details
Main Authors: Wang, Y., Uttarkar, P.A., Shannon, R.M., Lee, Y.W.J., Dobie, D., Wang, Andy, Bannister, K.W., Caleb, M., Deller, A.T., Glowacki, Marcin, Jahns-Schindler, J.N., Murphy, T., Anna-Thomas, R., Bhat, Ramesh, Deng, X., Gupta, V., Jaini, A., James, Clancy, Tuthill, J.
Format: Journal Article
Published: 2025
Online Access:http://hdl.handle.net/20.500.11937/97493

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