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- W4299346160 abstract "We have investigated the mass loss processes in Long Period Variables, by combining radiative transfer modeling with mid-IR imaging and spectroscopic observations. We find a correlation between variability type and temporal variations in the mass loss rate. Mira variables are more likely to maintain constant mass loss rates over long period of time. Semiregular and Irregular variables are characterized by frequent interruptions in their mass loss rate, on timescales of ~100 yr. High resolution imaging of individual Long Period Variable sources show departures from spherical symmetry. We present the case of o Cet (Mira), in which the presence of a low mass companion plays an active role in shaping the circumstellar environment." @default.
- W4299346160 created "2022-10-02" @default.
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- W4299346160 date "2002-04-09" @default.
- W4299346160 modified "2023-09-27" @default.
- W4299346160 title "An IR view of mass loss in Long Period Variables" @default.
- W4299346160 doi "https://doi.org/10.48550/arxiv.astro-ph/0204165" @default.
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