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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...

Ausführliche Beschreibung

Gespeichert in:
Hauptverfasser: Yuanming Wang, Pavan A. Uttarkar, Ryan M. Shannon, Yu Wing Joshua Lee, Dougal Dobie, Ziteng Wang, Keith W. Bannister, Manisha Caleb, Adam T. Deller, Marcin Glowacki, Joscha N. Jahns-Schindler, Tara Murphy, Reshma Anna-Thomas, N. D. R. Bhat, Xinping Deng, Vivek Gupta, Akhil Jaini, Clancy W. James, John Tuthill
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2025-01-01
Schriftenreihe:The Astrophysical Journal Letters
Schlagworte:
Pulsars
Radio pulsars
Radio transient sources
Online-Zugang:https://doi.org/10.3847/2041-8213/adbe61
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