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- W4241837984 abstract "The reports of periodic X–ray emission from the Seyfert galaxy NGC 6814 have motivated a number of exotic models for the active nucleus. Our ROSAT observation shows that while the nucleus of NGC 6814 is indeed an X–ray emitter, the periodicity is due to another source, most likely a Galactic accreting binary system, ∼ 37 arc min away." @default.
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- W4241837984 date "1994-01-01" @default.
- W4241837984 modified "2023-10-16" @default.
- W4241837984 title "Solving the Mystery of the Periodicity in the Seyfert Galaxy NGC 6814" @default.
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- W4241837984 doi "https://doi.org/10.1017/s0074180900174911" @default.
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