On the origins of part-time radio pulsars
Bing ZhangDepartment of Physics, University of Nevada, Las Vegas, NV 89154, USAJ. GilInstitute of Astronomy, Zielona Góra University, Lubuska 2, 65-265 Zielona Góra, PolandJ. DyksNicolaus Copernicus Centre, Polish Academy of Sciences, Torun, Poland
2006en
ABI
Abstract
Growing evidence suggests that some radio pulsars only act sporadically. These “parttime” pulsars include long-term nulls, quasi-periodic radio flares in PSR B1931+24, as well as the so-called Rotating RAdio Transients (RRATs). Based on the assumption
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