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    Wind Roche-Lobe overflow: a new mass-transfer mode for wide binaries by Mohamed, S, Podsiadlowski, P

    Published 2007
    “…Here we present preliminary simulations of a new mass-transfer mode - wind Roche-lobe overflow (RLOF) - that can occur when the wind acceleration region of the evolved star occurs at several stellar radii (as, e.g., in Mira variables). If this region is relatively close to the Roche-lobe, wind material fills the giant's Roche-lobe and is transferred to the hot component through the inner Lagrangian point (similar to standard RLOF). …”
    Conference item