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2001MNRAS.326L..33V - Mon. Not. R. Astron. Soc., 326, L33-L36 (2001/September-2)
Radio profile instability in the millisecond pulsar PSR J0437-4715 resulting from spiky emission.
VIVEKANAND M.
Abstract (from CDS):
The instability in one of the components of the radio integrated profile (IP) of the millisecond pulsar PSR J0437-4715 is correlated with the occurrence of the spiky emission in that component. It is speculated that the instability in other components is also as a result of the spiky emission. This might have important implications for interpreting the individual components of the IP as independent beams or regions of emission.
Abstract Copyright: The Royal Astronomical Society
Journal keyword(s): pulsars: general - pulsars: individual: PSR J0437-4715 - pulsars: individual: PSR B1821-24 - radio continuum: stars
Simbad objects: 2
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