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Glitches Vela pulsar

Next we compare Eq. (11) with an interpolation formula for the eight glitches of the Vela pulsar [16] ... [Pg.49]

Note that similar curves are obtained for the eight glitches of the Vela pulsar. As we see from Fig. 1, the behavior of AQ + AQ.S. is quite different in different parts of the relaxation region. The first part is the region of exponential relaxation with constants t and r2 and is located within the shell 9.533 < r < 9.61 km. The second part is the region of the exponential relaxation with t3 and linear relaxation, located within the shell 9.36 < r 5 9.533... [Pg.49]

Figure 1. The dependence of AO + AQ,S on the radius of the star for the first glitch of Vela pulsar. Figure 1. The dependence of AO + AQ,S on the radius of the star for the first glitch of Vela pulsar.
See other pages where Glitches Vela pulsar is mentioned: [Pg.44]    [Pg.45]    [Pg.47]    [Pg.48]    [Pg.49]    [Pg.51]   
See also in sourсe #XX -- [ Pg.48 ]



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Vela pulsar

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