Cargando…
On the Mass and Inclination of the PSR J2019+2425 Binary System
We report on nine years of timing observations of PSR J2019+2425, a millisecond pulsar in a wide 76.5 day orbit with a white dwarf. We measure a significant change over time of the projected semi-major axis of the orbit, x-dot/x=(1.3+-0.2)x10^-15 s^-1, where x=(a sin i)/c. We attribute this to the p...
Autores principales: | Nice, D J, Splaver, E M, Stairs, I H |
---|---|
Lenguaje: | eng |
Publicado: |
2001
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1086/319079 http://cds.cern.ch/record/471705 |
Ejemplares similares
-
Vacuum gaps in pulsars and PSR J2144-3933
por: Gil, J, et al.
Publicado: (2001) -
Discovery of PSR J0108-1431: the closest known neutron star?
por: Tauris, T M, et al.
Publicado: (1994) -
Binary Radio Pulsars
por: Fred Rasio, et al.
Publicado: (2005) -
Scintillation measurements of the millisecond pulsar PSR J0030+0451 and pulsar space velocities
por: Nicastro, L, et al.
Publicado: (2001) -
H.E.S.S.: Variable VHE gamma-Ray Emission from the Binary Pulsar PSR B1259-63
por: Schlenker, S
Publicado: (2005)