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- W2044201539 abstract "In a previous paper [1] we obtained statistically significant evidence for a 39-ms period in the COS-B data of 30–5000 MeV gamma rays in the direction of PSR 1951 + 32. Most of the gamma photons from PSR 1951 + 32 are pulsed and concentrated in a narrow interval of phase. We have examined the partical distribution of gamma ray intensity in the region around the pulsar and estimated the integrated flux to be 4.1 × 10−7 ph cm−2s−1 above 100 MeV and 8.2 × 10−8 ph cm−2s−1 above 300 MeV." @default.
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- W2044201539 date "1990-03-01" @default.
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- W2044201539 title "Pulsed gamma-rays from PSR 1951 + 32" @default.
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- W2044201539 doi "https://doi.org/10.1016/0275-1062(90)90003-v" @default.
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