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Table 2.

Examples illustrating the results of the parametric studies in Table 1 for pulsars with small companions.

Parameter Case B* R* P* r Rc Lnt σc fceo S Lsd iso, A iso, S τsd

Unit # T km ms AU km W mho GHz Jy W W W yr
Pulsar and asteroids

ϵ = 10−2, γ = 3 × 106, ΩA = 0.1 sr, T* = 5 × 105 K
Long P* 1 3.2 × 108 12 32 0.01 10 1025 102 28003 0.7 1.7 × 1032 9.0 × 1034 8.6 × 1034 381
Long P* 2 109 10 32 0.06 46 1027 107 1271 1.2 5.8 × 1032 1.6 × 1035 1.5 × 1035 114

ϵ = 10−2, γ = 3 × 106, ΩA = 0.1 sr, T* = 106 K
Low B*, σc 3 3.2 × 107 11 3 0.1 10 1027 102 212 0.4 1.0 × 1034 5.2 × 1034 5.0 × 1034 642
Small Rc 4 3.2 × 108 10 3 0.1 2 1027 107 1595 1.0 5.8 × 1035 1.4 × 1035 1.3 × 1035 11
Mild 5 3.2 × 108 12 10 0.1 10 1027 102 872 0.7 1.7 × 1034 8.8 × 1034 8.8 × 1034 38
Large Lnt 6 108 10 3 0.25 10 1028 107 80 0.3 5.8 × 1034 4.6 × 1034 4.5 × 1034 114
Large Lnt 7 3.2 × 108 10 3 0.63 10 1029 107 40 0.5 5.8 × 1035 7.3 × 1034 7.0 × 1034 11
Large S 8 3.2 × 108 10 3 0.1 10 1027 102 1595 22. 5.8 × 1035 3.0 × 1036 2.8 × 1036 11
Large r 9 108 12 3 0.4 10 1027 107 54 0.4 1.7 × 1035 5.5 × 1034 5.3 × 1034 38

ϵ = 10−2, γ = 3 × 106, ΩA = 1 sr, T* = 106 K
Large r 10 3.2 × 108 10 3 0.16 10 1027 102 633 0.9 5.8 × 1035 1.2 × 1035 1.1 × 1035 11
Low B* 11 108 11 3 0.1 10 1027 107 671 0.4 1.0 × 1035 5.2 × 1034 5.0 × 1034 64

ϵ = 2 × 10−3, γ = 106, ΩA = 0.1 sr, T* = 106 K
Low γ 12 3.2 × 108 10 3 0.1 10 1027 107 532 0.5 5.8 × 1035 6.6 × 1034 6.3 × 1034 11

ϵ = 2 × 10−3, γ = 3 × 106, ΩA = 0.1 sr, T* = 106 K
Long τsd 13 108 10 3 0.1 10 1027 107 504 0.4 5.8 × 1034 5.9 × 1034 5.7 × 1034 114
Large S, τsd 14 3.2 × 107 10 3 0.025 100 1025 107 2552 71. 5.8 × 1033 9.4 × 1036 9.0 × 1036 1138
Huge S 15* 108 10 3 0.025 316 1025 102 8071 7 × 103 5.8 × 1034 9.4 × 1038 9.0 × 1038 114

Magnetar and asteroids

ϵ = 10−2, γ = 3 × 106, ΩA = 0.1 sr, T* = 2.×106 K
Small Rc 16 1010 10 100 0.1 46 1027 10 1595 0.5 5.8 × 1032 6.4 × 1034 6.1 × 1034 11.4

Notes. Input parameters are provided in the upper line (above the double line). We abbreviate the maximum admissible value of (1 − f)gLsd as Lnt.

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