LOFAR discovery of a quiet emission mode in PSR B0823+26

C G Sobey, N J Young,J W T Hessels,P Weltevrede,A Noutsos,B W Stappers,M J Kramer,C G Bassa,A G Lyne,V I Kondratiev,T E Hassall,E F Keane,A V Bilous,R P Breton, J M Griesmeier,A Karastergiou,M Pilia, M Serylak,S Ter Veen, J Van Leeuwen,A Alexov,J M Anderson,A Asgekar,I M Avruch,M E Bell,M J Bentum,G Bernardi,P N Best, L Birzan,A Bonafede,F Breitling,J W Broderick,M Bruggen,A Corstanje,D Carbone,E De Geus,M De Vos,A Van Duin,S Duscha,Jochen Eisloffel,H Falcke,R A Fallows,R P Fender,C Ferrari,W Frieswijk,M A Garrett,A W Gunst, J P Hamaker,G Heald,M Hoeft, J R Horandel, E Jutte,G Kuper,P Maat,Giovanni E Mann,Sera Markoff,R Mcfadden, D Mckaybukowski,J P Mckean,D D Mulcahy,H Munk,A Nelles, M J Norden, E Orru,H Paas,M Pandeypommier,V N Pandey, G Pietka, R Pizzo,A G Polatidis, D A Rafferty, A Renting,H J A Rottgering,A Rowlinson, Anna M M Scaife,Dominik J Schwarz,J Sluman,O Smirnov,Michael P Steinmetz,Alexandre F R Stewart,J Swinbank,Michel Tagger,Yu Tang,C Tasse,S Thoudam, C Toribio, R C Vermeulen, C Vocks,R J Van Weeren,R A M J Wijers,M W Wise,O Wucknitz,S Yatawatta, P Zarka

Monthly Notices of the Royal Astronomical Society（2015）

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摘要

PSR B0823+26, a 0.53-s radio pulsar, displays a host of emission phenomena over time-scales of seconds to (at least) hours, including nulling, subpulse drifting, and mode-changing. Studying pulsars like PSR B0823+26 provides further insight into the relationship between these various emission phenomena and what they might teach us about pulsar magnetospheres. Here we report on the LOFAR (Low-Frequ...

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关键词

stars: neutron,pulsars: individual: PSR B0823+26

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