Evidence for geodetic spin precession in the binary pulsar 1913 + 16

1989 ◽  
Vol 347 ◽  
pp. 1030 ◽  
Author(s):  
J. M. Weisberg ◽  
R. W. Romani ◽  
J. H. Taylor
1988 ◽  
Vol 49 (C6) ◽  
pp. C6-17-C6-22 ◽  
Author(s):  
Z. HUANG ◽  
P. H. CUTLER ◽  
T. E. FEUCHTWANG ◽  
R. H. GOOD ◽  
Jr. ◽  
...  

1996 ◽  
Vol 165 ◽  
pp. 313-319
Author(s):  
Mark H. Finger ◽  
Robert B. Wilson ◽  
B. Alan Harmon ◽  
William S. Paciesas

A “giant” outburst of A 0535+262, a transient X-ray binary pulsar, was observed in 1994 February and March with the Burst and Transient Source Experiment (BATSE) onboard the Compton Gamma-Ray Observatory. During the outburst power spectra of the hard X-ray flux contained a QPO-like component with a FWHM of approximately 50% of its center frequency. Over the course of the outburst the center frequency rose smoothly from 35 mHz to 70 mHz and then fell to below 40 mHz. We compare this QPO frequency with the neutron star spin-up rate, and discuss the observed correlation in terms of the beat frequency and Keplerian frequency QPO models in conjunction with the Ghosh-Lamb accretion torque model.


Author(s):  
Seong Been Kim ◽  
Jeehoon Jeon ◽  
Hyung-jun Kim ◽  
Joonyeon Chang ◽  
Hyun Cheol Koo

1989 ◽  
Author(s):  
I. A. Koop ◽  
A. P. Lysenko ◽  
I. N. Nesterenko ◽  
A. A. Polunin ◽  
Yu. M. Shatunov
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