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• W2164320268 abstract "We report on ASCA, RXT E, and archival observations of the high-mass X-ray binary pulsar 4U 1907]09. Spectral measurements of the absorption and —ux were made at all phases of the X-ray pulsar orbit, including the —rst spectral measurements of an extended period of low —ux during two of the ASCA observations. We —nd that a simple spherical wind model can —t the time-averaged light curve as measured by the RXT E All-Sky Monitor but does not —t the observed changes in the absorption column or account for the existence of the phase-locked secondary —are. An additional model component consisting of a trailing stream can account for the variations in column depth. However, these models favor a high inclination angle for the system, suggesting a companion mass more consistent with an identi—cation as a Be star. In this case, an equatorially enhanced wind and inclined neutron star orbit may be a more appropriate interpretation of the data." @default.
• W2164320268 created "2016-06-24" @default.
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• W2164320268 date "2001-07-10" @default.
• W2164320268 modified "2023-10-18" @default.
• W2164320268 title "Phase‐dependent Spectral Variability in 4U 1907+09" @default.
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• W2164320268 doi "https://doi.org/10.1086/321487" @default.
• W2164320268 hasPublicationYear "2001" @default.
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