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- W2020560585 abstract "The close (P == 0.7 day) synchronized binary system ER Vul was observed 4 times for 11.5 hours with the VLA system: twice in 1990, mostly at 6 cm with some data at 20 cm, and twice in 1991, mostly at 3.6 cm. The C- and X-band radio light-curves revealed complex variability, a mixture of the slow (geometrical and/or slow magnetic structure evolution) and of the random (flaring) components. The expected rigid anchoring of the emitting structures to the binary system geometry was not observed. The 6 cm data showed a semi-periodicity of about 0.8 day whereas the 3.6 cm data seemed to indicate more short time-scale (flaring) variability which was modulated by the half-day visibility window at daily intervals. The flux levels were very similar at 3.6 and 6 cm in 1991 but were lower at 20 cm than at 6 cm in 1990 data. There was an appreciable decrease in the 6 cm flux level between 1990 and 1991. No appreciable (> 5 sigma) circular polarization was observed at any time." @default.
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- W2020560585 date "1992-12-01" @default.
- W2020560585 modified "2023-10-18" @default.
- W2020560585 title "VLA radio light curves of ER Vulpeculae at 3.6 and 6 CM" @default.
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- W2020560585 doi "https://doi.org/10.1086/133106" @default.
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