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Galactic Gamma‐Ray Background as a Constraint on Millisecond Pulsars
Bhatia et al. 1997 The Astrophysical Journal 476 238.
Caption: Fig. 5.
Expected γ‐ray flux from the millisecond pulsars in the outer Galaxy (longitude range 60°–300°). COS B observations are also shown.
© 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.