Diffractive Scintillation of the Pulsar PSR B1259−63

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Diffractive Scintillation of the Pulsar PSR B1259-63

PSR B1259–63 is in a highly eccentric 3.4 yr orbit around the Be-star SS2883. The system is located in the direction of the Sagittarius-Carina spiral arm at a distance of ∼1.5 kpc. We have made scintillation observations of the pulsar far from periastron at 4.8 GHz and 8.4 GHz, determining the diffractive bandwidth, ∆νd, and timescale, ∆td, at both frequencies. We find no dependency on orbital ...

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 1998

ISSN: 0004-637X

DOI: 10.1086/311088