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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. 3.
Same as Fig. 2, except that the average number of millisecond pulsars per globular cluster assumed is 1500
© 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.
