Astronomy and Astrophysics – Astrophysics
Scientific paper
1997-10-21
ApJ 491 (1997) L95
Astronomy and Astrophysics
Astrophysics
10 pages, 2 figures, to appear in Astrophys. J. Lett
Scientific paper
10.1086/311060
Using recently calculated analytic and numerical models for the thermal structure of ultramagnetized neutron stars, we estimate the effects that ultrastrong magnetic fields $B \ge 10^{14}$ G have on the thermal evolution of a neutron star. Understanding this evolution is necessary to interpret models that invoke ``magnetars'' to account for soft $\gamma$-ray emission from some repeating sources.
Hernquist Lars
Heyl Jeremy S.
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