Fig. 1 from Joule Heating and the Thermal Evolution of Old Neutron Stars

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Joule Heating and the Thermal Evolution of Old Neutron Stars

Authors: Juan A. Miralles, Vadim Urpin, and Denis Konenkov

Miralles, Urpin, & Konenkov 1998 The Astrophysical Journal 503 368.

Provider: AAS Journals

Caption: Fig. 1.

Time dependence of the rate of Joule heating integrated over the star volume and normalized to B_e13 = B_e/10¹³ G. Numbers near the curves indicate the logarithm of ρ₀. Different types of lines correspond to different values of ξ: 0.1 (solid line), 0.01 (dashed line), 0.001 (dotted line).

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