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- W132103553 abstract "We have produced a movie of the time evolution of the v=1, J=1−0 43 GHz SiO masers in the inner circumstellar envelope of the isolated Mira variable TX Cam. Our observations, taken every two weeks with the VLBA, currently cover about 60% of the stellar cycle from ϕ ∼ 0.6 → ϕ ∼ 1.2. They show that, in contrast to previous observations and theoretical models, the gas in which the masers are embedded is undergoing expansion during this period with a typical velocity of 3.65 ± 0.15 km/s. Some isolated features are seen to start falling back towards the star at around ϕ ∼ 1.0. We suggest that the 5 → 10 G magnetic fields we have previously detected at the position of the SiO masers may explain the departure from the expected behaviour." @default.
- W132103553 created "2016-06-24" @default.
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- W132103553 date "1999-01-01" @default.
- W132103553 modified "2023-09-24" @default.
- W132103553 title "Making movies of stars: VLBA monitoring of the SiO masers around the Mira variable TX Cam" @default.
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- W132103553 doi "https://doi.org/10.1017/s0074180900203070" @default.
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