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| Query : 2001MNRAS.326L..33V |
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
| Number of rows : 2 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | PSR J0437-47 | Psr | 04 37 15.7994581776 | -47 15 08.544351636 | DC | 1032 | 0 | |||||
| 2 | PSR J1824-2452A | Psr | 18 24 32.009 | -24 52 11.10 | ~ | 529 | 2 |
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