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- W2101784423 abstract "Abstract The 7 s X-ray pulsar 1E 2259+586 and the supernova remnant (SNR) G109.1-1.0 (CTB 109) were observed by BeppoSAX in 1996 November. We confirm the ASCA discovery of an additional low-energy spectral component from 1E2259+586. This can be modeled as a 0.44 keV blackbody, but we cannot exclude that some, or all, of this emission arises from the part of the SNR that lies within the pulsar's extraction region. The G109.1-1.0 spectrum is well fit with a non-equilibrium ionization plasma model with a best-fit temperature of 0.95 keV. The derived mass for the X-ray emitting plasma (∼15–20 M ⊙ ) and its near cosmic abundances imply that the X-ray emission comes mainly from mildly enriched, swept-up circumstellar material. The spectrum is strongly out of equilibrium with an ionization age of only 3000 yr." @default.
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- W2101784423 date "1999-01-01" @default.
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- W2101784423 title "An X-ray spectroscopic study of the pulsar 1E2259+586 and the supernova remnant G109.1-1.0 (CTB 109)" @default.
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- W2101784423 doi "https://doi.org/10.1016/s0920-5632(98)00191-1" @default.
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