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- W2100806313 abstract "We study the possibility that the very broad (∼1500 km s−1) and luminous (L5007∼ 1.4 × 1037 erg s−1) [O iii] line emission observed in the globular cluster RZ 2109 might be explained with the photoionization of nova ejecta by the bright (LX∼ 4 × 1039 erg s−1) X-ray source hosted in the same globular cluster. We find that such scenario is plausible and explains most of the features of the RZ 2109 spectrum (line luminosity, absence of H emission lines, peculiar asymmetry of the line profile); on the other hand, it requires the nova ejecta to be relatively massive (≳0.5 × 10−3 M⊙), and the nova to be located at a distance ≲0.1 pc from the X-ray source. We also predict the time evolution of the RZ 2109 line emission, so that future observations can be used to test this scenario." @default.
- W2100806313 created "2016-06-24" @default.
- W2100806313 creator A5071822154 @default.
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- W2100806313 date "2012-05-01" @default.
- W2100806313 modified "2023-10-06" @default.
- W2100806313 title "Broad [O iii] in the globular cluster RZ 2109: X-ray ionized nova ejecta" @default.
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- W2100806313 doi "https://doi.org/10.1111/j.1365-2966.2012.20942.x" @default.
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