scholarly journals Gamma-rays from accretion process onto millisecond pulsars

2016 ◽  
Author(s):  
Wlodek Bednarek
Keyword(s):  
Gamma Rays ◽  
Millisecond Pulsars ◽  
Accretion Process

Gamma rays from millisecond pulsars

1991 ◽  
Vol 12 (1) ◽  
pp. 17-25 ◽  
Author(s):  
D. Bhattacharya ◽  
G Srinivasan
Keyword(s):  
Gamma Rays ◽  
Millisecond Pulsars

scholarly journals Pulsars in gamma rays: What Fermi is teaching us

2012 ◽  
Vol 8 (S291) ◽  
pp. 307-312 ◽  
Author(s):  
Matthew Kerr ◽  
Keyword(s):  
Neutron Star ◽  
Gamma Rays ◽  
Large Population ◽  
Radiation Mechanism ◽  
Millisecond Pulsars ◽  
Universal Properties ◽  
Γ Ray

AbstractThe 2nd Fermi-LAT pulsar catalog includes 117 γ-ray pulsars, of which roughly one third are millisecond pulsars (MSPs) while the remaining two thirds split evenly into young radio-loud and radio-quiet pulsars. Although this large population will enable future, detailed studies of emission mechanisms and the evolution of the underlying neutron star population, some nearly-universal properties are already clear and unequivocal. We discuss some of these aspects below, including the altitude of the γ-ray emission site, the shape of the γ-ray spectrum, and the implications of the latter for the radiation mechanism.

scholarly journals Discovery and Timing of Three Millisecond Pulsars in Radio and Gamma-Rays with the Giant Metrewave Radio Telescope and Fermi Large Area Telescope

2021 ◽  
Vol 910 (2) ◽  
pp. 160
Author(s):  
B. Bhattacharyya ◽  
J. Roy ◽  
T. J. Johnson ◽  
P. S. Ray ◽  
P. C. C. Freire ◽  
...  
Keyword(s):  
Radio Telescope ◽  
Gamma Rays ◽  
Large Area ◽  
Millisecond Pulsars

TeV gamma rays from millisecond pulsars

1991 ◽  
Author(s):  
C. C. G. Bowden ◽  
S. M. Bradbury ◽  
K. T. S. Brazier ◽  
A. Carramiñana ◽  
P. M. Chadwick ◽  
...  
Keyword(s):  
Gamma Rays ◽  
Millisecond Pulsars ◽  
Tev Gamma Rays

scholarly journals The maximum spin of Millisecond Pulsar and the gravitational wave

2015 ◽  
Vol 11 (A29B) ◽  
pp. 370-371
Author(s):  
C. M. Zhang
Keyword(s):  
Neutron Star ◽  
Gravitational Wave ◽  
Wave Radiation ◽  
Millisecond Pulsar ◽  
Millisecond Pulsars ◽  
Accretion Process ◽  
Maximum Spin

AbstractThe gravitational wave radiation will release the energy momentum, which will dissipate the rotation of neutron star while in the accretion process. If the deformation of star is known, then we can estimate the maximum spin frequency of pulsar, based on which we can interpret why the spin periods of all millisecond pulsars cannot be less than one millisecond.

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