Issue 
A&A
Volume 574, February 2015



Article Number  A77  
Number of page(s)  32  
Section  Stellar structure and evolution  
DOI  https://doi.org/10.1051/00046361/201424672  
Published online  28 January 2015 
Online material
Appendix A: Physical quantity maps for different clump parameters
The density zoom, tracer, pressure, ratio of momentumflux 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
Zoomin 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 threevelocity at different locations (β = v/c). The axes units are a = 8 × 10^{10} 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 ρ_{0}c^{2} 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 Γ^{2}v^{2}(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
Zoomin 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. 

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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. 

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Fig. A.8
Pressure distribution in units of ρ_{0}c^{2} 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. 

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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 Γ^{2}v^{2}(1 + ϵ + P/ρ) + P. The remaining plot properties are the same as those of Fig. A.1. 

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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. 

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Fig. A.11
Zoomin 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. 

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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. 

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Fig. A.13
Pressure distribution in units of ρ_{0}c^{2} 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. 

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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 Γ^{2}v^{2}(1 + ϵ + P/ρ) + P. The remaining plot properties are the same as those of Fig. A.1. 

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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. 

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© ESO, 2015
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