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• W1578129675 abstract "A new X-ray source, XTE J1855-026, was discovered during Rossi X-Ray Timing Explorer (RXTE) scans along the Galactic plane. The source shows pulsations at a period of 361 s and also modulation at a period of 6.1 days, which we interpret as the orbital period of the system. The X-ray spectrum above ~3 keV can be fitted with an absorbed power-law model with a high-energy cutoff and an iron emission line at approximately 6.4 keV. We interpret these results as indicating that XTE J1855-026 is likely to consist of a neutron star accreting from the wind of an O or B supergiant primary. A less likely interpretation is that XTE J1855-026 is instead a Be/neutron star binary, in which case it would have the shortest known orbital period for such a system." @default.
• W1578129675 created "2016-06-24" @default.
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• W1578129675 date "1999-06-01" @default.
• W1578129675 modified "2023-10-03" @default.
• W1578129675 title "<i>Rossi X‐Ray Timing Explorer</i>Observations of the X‐Ray Pulsar XTE J1855−026: A Possible New Supergiant System" @default.
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• W1578129675 doi "https://doi.org/10.1086/307235" @default.
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