Fig. 6 from Galactic Gamma‐Ray Background as a Constraint on Millisecond Pulsars

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Galactic Gamma‐Ray Background as a Constraint on Millisecond Pulsars

Authors: V. B. Bhatia, S. Misra, and and N. Panchapakesan

Bhatia et al. 1997 The Astrophysical Journal 476 238.

Provider: AAS Journals

Caption: Fig. 6.

The expected γ‐ray flux from the disk component of millisecond pulsars (10⁴ in number) (Curve 1), supplementing the predictions of Strong et al. (1988), is shown as Curve 2. COS B observations are also shown.

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