THE STRONG MAGNETIC FIELD DECAY AND EVOLUTION OF RADIO PULSARS ON THE P–Ṗ DIAGRAM
OKTAY H. GUSEINOVAkdeniz University, Physics Department, Antalya, TurkeyAŞKIN ANKAYTÜBİTAK Feza Gürsey Institute, 81220 Çengelköy, İstanbul, TurkeySEVINÇ O. TAGIEVAAcademy of Science, Physics Institute, Baku 370143, Azerbaijan Republic
2004en
ABI
Аннотация
In this work we have analysed various data on radio pulsars and we have shown that magnetic field decay of a factor about 10–20 is necessary to explain their evolution, in particular to remove the discrepancy between the characteristic and the real ages. The character of the field decay is exponential with a characteristic time of about 3×10 6 year. Observational data on single X-ray pulsars which radiate due to cooling also support this result.
Ҳали таржима қилинмаган
Идентификаторлар
Иқтибослар ва манбалар
2 та иқтибос0 та фойдаланилган манба