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Table 4

Upper limits of the dust mass-loss rate r per mass bins and velocity vr at the heliocentric distances r (AU) before perihelion.

Δmcompact Δmfluffy 3.4 v3.4 3.2 v3.2 3.0 v3.0 2.6 v2.6 1.9 v1.9 1.3 v1.3
kg kg kg s-1 m s-1 kg s-1 m s-1 kg s-1 m s-1 kg s-1 m s-1 kg s-1 m s-1 kg s-1 m s-1

E+00-E+01 E+02-E+03 60 0.5 120 0.7
E-01-E+00 E+01-E+02 45 0.7 60 0.8 120 1
E-02-E-01 E+00-E+01 20 0.7 45 1 60 1.1 120 1.5
E-03-E-02 E-01-E+00 5.0 0.7 20 1 45 1.5 60 1.6 120 2.1
E-04-E-03 E-02-E-01 5.0 1 20 1.5 45 2.1 60 2.4 120 3.2
E-05-E-04 E-03-E-02 5.0 1.5 20 2.1 45 3.2 60 3.5 120 4.7
E-06-E-05 E-04-E-03 4.0 2.1 16 3.2 30 4.7 45 5.1 100 6.6
E-07-E-06 E-05-E-04 2.0 3.2 8.0 4.7 15 6.6 22 7.6 65 10
E-08-E-07 E-06-E-05 1.2E-1 0.7 1.0 4.7 4.0 6.6 7.5 10 11 11 48 15
E-09-E-08 E-07-E-06 6.0E-2 1 5.0E-1 6.6 2.0 10 3.7 15 5.5 16 33 21
E-10-E-09 E-08-E-07 3.0E-2 1.5 2.5E-1 10 1.0 15 1.8 21 2.7 24 21 32
E-11-E-10 E-09-E-08 1.5E-2 2.1 1.2E-1 15 5.0E-1 21 9.0E-1 32 1.3 35 12 47
E-12-E-11 E-10-E-09 7.5E-3 3.2 6.0E-2 21 2.5E-1 32 4.5E-1 47 6.5E-1 52 9.0 66
E-13-E-12 E-11-E-10 3.7E-3 4.7 3.0E-2 32 1.2E-1 47 2.2E-1 66 3.2E-1 76 6.0 100
E-14-E-13 E-12-E-11 1.8E-3 6.6 1.5E-2 47 6.0E-2 66 1.1E-1 100 1.6E-1 110 4.5 150
E-15-E-14 E-13-E-12 9.0E-4 10 7.7E-3 66 3.0E-2 100 5.5E-2 150 8.0E-2 160 3.3 210

Notes. The mass-loss rates are computed assuming Ap = 0.02, the Afρ-curve plotted in Fig. 13 and an escape velocity at the end of the gas drag of 0.5 m s-1.

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