V

A = 0

A = 0.2

A = 0.4

A = 0.8

A = 1.6

A = 3.2

1.3E+15

1.1E+15

9.0E+14

6.0E+14

2.7E+14

5.5E+13

10°

2.6E+14

2.1E+14

1.7E+14

1.2E+14

5.3E+13

1.1E+13

45°

5.0E+13

4.1E+13

3.4E+13

2.3E+13

1.1E+13

2.3E+12

90°

2.4E+13

2.0E+13

1.6E+13

1.1E+13

5.3E+12

1.2E+12

178°

1.5E+13

1.2E+13

1.0E+13

7.2E+12

3.5E+12

8.7E+11

1.14.6. Gamma ray fluxes from stellar winds

In this case robs >> ro, and the expected gamma ray fluxes will be n 2

Y((,robs, t)= 1.45 X2nrobs Jcos 00 Jr2F^ ((,r,0, t)

•9n ro"b2s fYh E rfrJ (b, a(ey , t) (1.14.29)

where

v v li 1 A ) u2 (1 A , + b\— + — + ... I + b2\ -+ —+... | +...

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