scholarly journals AstroSat observation of the Be/X-ray binary Pulsar 3A 0726-260 (4U 0728-25)

2020 ◽  
Vol 20 (9) ◽  
pp. 155
Author(s):  
Jayashree Roy ◽  
Prahlad C. Agrawal ◽  
Baibhav Singari ◽  
Ranjeev Misra
Keyword(s):  
X Ray ◽  
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.


2008 ◽  
Vol 387 (2) ◽  
pp. 724-728 ◽  
Author(s):  
M. J. Coe ◽  
M. Schurch ◽  
R. H. D. Corbet ◽  
J. Galache ◽  
V. A. McBride ◽  
...  

1992 ◽  
Vol 401 ◽  
pp. 685 ◽  
Author(s):  
N. R. Robba ◽  
G. Cusumano ◽  
M. Orlandini ◽  
D. dal Fiume ◽  
F. Frontera
Keyword(s):  
X Ray ◽  

1992 ◽  
Vol 386 ◽  
pp. 703 ◽  
Author(s):  
Mauro Orlandini ◽  
G. E. Morfill
Keyword(s):  
X Ray ◽  

Author(s):  
V. A. Torres-Sánchez ◽  
E. Contreras

Abstract In this work we obtain an anisotropic neutron star solution by gravitational decoupling starting from a perfect fluid configuration which has been used to model the compact object PSR J0348+0432. Additionally, we consider the same solution to model the Binary Pulsar SAX J1808.4-3658 and X-ray Binaries Her X-1 and Cen X-3 ones. We study the acceptability conditions and obtain that the MGD-deformed solution obey the same physical requirements as its isotropic counterpart. Finally, we conclude that the most stable solutions, according to the adiabatic index and gravitational cracking criterion, are those with the smallest compactness parameters, namely SAX J1808.4-3658 and Her X-1.


2016 ◽  
Vol 457 (3) ◽  
pp. 2749-2760 ◽  
Author(s):  
Gaurava K. Jaisawal ◽  
Sachindra Naik ◽  
Prahlad Epili
Keyword(s):  
Type I ◽  
X Ray ◽  

2015 ◽  
Vol 15 (4) ◽  
pp. 537-548 ◽  
Author(s):  
Sachindra Naik ◽  
Gaurava K. Jaisawal
Keyword(s):  
X Ray ◽  

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