Astrophysics - download pdf or read online

By G. Borner, J. Stewart

ISBN-10: 0387063765

ISBN-13: 9780387063768

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The models obtained are non-rotating and since pulsars are presently believed to be rotating neutron stars, further information is needed. As will be seen below, typical neutron stars have a radius only a few times their gravitational radius. Thus, general relativistic effects are quite important and must be taken into account. One such general relativistic effect is the dragging along of inertial frames by rotating bodies (Brill and Cohen, 1966; Cohen, 1965). Unlike in Newtonian mechanics, where a gyroscope points towards the same distant star independent of the motion of nearby masses, rotating masses in general relativity drag along the inertial frames and cause the rotation axis of a gyroscope to precess.

2 378 396 40 G. Bfrner: Table 6 (B6rner and Cohen, 1973) gives the crust's moment of inertia and that of the entire star vs. central density. , 1971 b). 3. The Crab Pulsar The Crab pulsar is located at the center of the Crab nebula, the remnant of a supernova that exploded in 1054. Because of its location in the nebula a distance estimate independent of the pulsar's dispersion can be obtained. 5 kpc cannot be excluded. Let us, however, be definite and adopt a distance of 2 kpc for the Crab Nebula.

Ff the shell is pushed out by low-frequency waves from the pulsar, and if according to Gunn and Ostriker (1969) protons get ten times the energy of the electrons, then only the maximum mass (near the mass peak) neutron star models of the CCLR equation of state can fulfill this requirement, as indicated by line (d) in Fig. 6. This particle acceleration mechanism therefore seems to be unrealistic. If the distance to the Crab were less or more than 2 kpc, the limits derived above would have to be scaled down or up accordingly.

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Astrophysics by G. Borner, J. Stewart

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