Simulations of an inhomogeneous stellar wind interacting with a pulsar wind in a binary system

Free Access

Issue		A&A Volume 574, February 2015


Article Number		A77
Number of page(s)		32
Section		Stellar structure and evolution
DOI		https://doi.org/10.1051/0004-6361/201424672
Published online		28 January 2015

Online material

Appendix A: Physical quantity maps for different clump parameters

The density zoom, tracer, pressure, ratio of momentum-flux to pressure, and velocity maps are presented in Figs. A.1–A.15 for different clump parameters: χ = 10 and R_c = 1 a; χ = 10 and R_c = 5 a; and χ = 30 and R_c = 1 a.

	Fig. A.1 Zoom-in of the density distribution by colour for the case with clump parameters χ = 10 and R_c = 1 a for the times shown at the top of each plot. The coloured arrows represent the three-velocity at different locations (β = v/c). The axes units are a = 8 × 10¹⁰ cm. The pulsar and the star are located at (r,z) = (0,5 a) and (r,z) = (0,60 a), respectively.
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	Fig. A.2 Tracer distribution by colour for the case with clump parameters χ = 10 and R_c = 1 a for the times shown at the top of each plot. The tracer value ranges from 0 (pulsar and stellar wind) to 1 (clump). The remaining plot properties are the same as those of Fig. A.1.
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	Fig. A.3 Pressure distribution in units of ρ₀c² by colour for the case with clump parameters χ = 10 and R_c = 1 a for the times shown at the top of each plot. The remaining plot properties are the same as those of Fig. A.1.
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	Fig. A.4 Momentum flux over pressure distribution by colour for the case with clump parameters χ = 10 and R_c = 1 a for the times shown at the top of each plot. The momentum flux is given by F_p = ρ Γ²v²(1 + ϵ + P/ρ) + P. The remaining plot properties are the same as those of Fig. A.1.
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	Fig. A.5 β distribution by colour for the case with clump parameters χ = 10 and R_c = 1 a for the times shown at the top of each plot. The remaining plot properties are the same as those of Fig. A.1.
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	Fig. A.6 Zoom-in of the density distribution by colour for the case with clump parameters χ = 10 and R_c = 5 a for the times shown at the top of each plot. The remaining plot properties are the same as those of Fig. A.1.
Open with DEXTER

	Fig. A.7 Tracer distribution by colour for the case with clump parameters χ = 10 and R_c = 5 a for the times shown at the top of each plot. The tracer value ranges from 0 (pulsar and stellar wind) to 1 (clump). The remaining plot properties are the same as those of Fig. A.1.
Open with DEXTER

	Fig. A.8 Pressure distribution in units of ρ₀c² by colour for the case with clump parameters χ = 10 and R_c = 5 a for the times shown at the top of each plot. The remaining plot properties are the same as those of Fig. A.1.
Open with DEXTER

	Fig. A.9 Momentum flux over pressure distribution by colour for the case with clump parameters χ = 10 and R_c = 5 a for the times shown at the top of each plot. The momentum flux is given by F_p = ρ Γ²v²(1 + ϵ + P/ρ) + P. The remaining plot properties are the same as those of Fig. A.1.
Open with DEXTER

	Fig. A.10 β distribution by colour for the case with clump parameters χ = 10 and R_c = 5 a for the times shown at the top of each plot. The remaining plot properties are the same as those of Fig. A.1.
Open with DEXTER

	Fig. A.11 Zoom-in of the density distribution by colour for the case with clump parameters χ = 30 and R_c = 1 a for the times shown at the top of each plot. The remaining plot properties are the same as those of Fig. A.1.
Open with DEXTER

	Fig. A.12 Tracer distribution by colour for the case with clump parameters χ = 30 and R_c = 1 a for the times shown at the top of each plot. The tracer value ranges from 0 (pulsar and stellar wind) to 1 (clump). The remaining plot properties are the same as those of Fig. A.1.
Open with DEXTER

	Fig. A.13 Pressure distribution in units of ρ₀c² by colour for the case with clump parameters χ = 30 and R_c = 1 a for the times shown at the top of each plot. The remaining plot properties are the same as those of Fig. A.1.
Open with DEXTER

	Fig. A.14 Momentum flux over pressure distribution by colour for the case with clump parameters χ = 30 and R_c = 1 a for the times shown at the top of each plot. The momentum flux is given by F_p = ρ Γ²v²(1 + ϵ + P/ρ) + P. The remaining plot properties are the same as those of Fig. A.1.
Open with DEXTER

	Fig. A.15 β distribution by colour for the case with clump parameters χ = 30 and R_c = 1 a for the times shown at the top of each plot. The remaining plot properties are the same as those of Fig. A.1.
Open with DEXTER

© ESO, 2015

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