Fig. 7 from Inferring the Spatial and Energy Distribution of Gamma‐Ray Burst Sources. III. Anisotropic Models

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Inferring the Spatial and Energy Distribution of Gamma‐Ray Burst Sources. III. Anisotropic Models

Authors: Thomas J. Loredo and Ira M. Wasserman

Loredo & Wasserman 1998 The Astrophysical Journal 502 108.

Provider: AAS Journals

Caption: Fig. 7.

Visibility of large Galactocentric shells. Only the highlighted part of a Galactocentric shell of radius r is visible, if r is comparable to the maximum solarcentric radius r^{﹩\arcmin﹩}, from which bursts are visible. The visible portion has a large negative dipole moment.

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