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- W1626509584 abstract "From five-colour photometry of the triple-periodic systems H2252-035 and V1223 Sgr, which have very similar orbital and pulsation periods, we find a significant difference in the wavelength dependence of their short period pulsations. Our results indicate that in H2252-035 this pulse originates in a hot region, probably on the white dwarf (Motch and Pakull, 1981), whereas in V1223 Sgr both pulses are the result of reprocessing of X-rays (in the far side of the accretion disk, and in the companion star, respectively), as suggested by Warner (1985)." @default.
- W1626509584 created "2016-06-24" @default.
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- W1626509584 date "1985-01-01" @default.
- W1626509584 modified "2023-10-03" @default.
- W1626509584 title "A Comparison of H2252-035/AO PSC and 4U1849-31/V1223 SGR" @default.
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- W1626509584 doi "https://doi.org/10.1007/978-94-009-5319-2_32" @default.
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