Fig. 3 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. 3.

Thermal evolution of the PS model with and without Joule heating. Curve 1: B_e = 1.5 × 10¹³ G, ρ₀ = 10¹³ g cm⁻³, ξ = 0.1. Curve 2: B_e = 1.5 × 10¹³ G, ρ₀ = 5 × 10¹² g cm⁻³, ξ = 0.1. Curve 3: B_e = 1.5 × 10¹³ G, ρ₀ = 10¹³ g cm⁻³, ξ = 0.01. Curve 4: B_e = 5 × 10¹² G, ρ₀ = 10¹³ g cm⁻³, ξ = 0.1. Curve 5: without Joule heating.

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