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- W2007276070 abstract "view Abstract Citations (4) References (10) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS A new X-ray pulsar with a 67-millisecond period in the constellation Equuleus Sadeh, D. ; Livio, M. Abstract On November 18 and 19, 1977, the large area detector on the HEAO satellite pointed for 96 minutes toward one direction. At that time the 5-ms mode was employed, and 5-ms data accumulations were transmitted. Some 753,000 data points were epoch-folded to search for periods between 10 ms and 100 ms, and one period showed a very low expectation for random occurrences. This point was persistent for a long enough time to permit the epoch-folding of a large body of data, its precise determination to 0.1 microsec, and the sighting of its light curve. All the tests performed indicate the existence of a pulsar in this place. The period of this pulsar is 67.5492 ms, corrected for heliocentric coordinates (its local period is 67.55328 ms). Its expectation for random occurrence is lower than 5 x 10 to the -9th. Publication: The Astrophysical Journal Pub Date: December 1982 DOI: 10.1086/160552 Bibcode: 1982ApJ...263..823S Keywords: Heao 1; Light Curve; Pulsars; Spaceborne Astronomy; X Ray Sources; Neutron Stars; Statistical Analysis; Stellar Magnetic Fields; Stellar Rotation; Astronomy full text sources ADS |" @default.
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- W2007276070 title "A new X-ray pulsar with a 67-millisecond period in the constellation Equuleus" @default.
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