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• W2890461387 abstract "We study the grazing envelope evolution (GEE), where a secondary star, which orbits the surface of a giant star, accretes mass from the giant envelope and launches jets. We conduct simulations of the GEE with different half-opening angles and velocities, and simulate the onset phase and the spiralling-in phase. We discuss the resulting envelope structure and the outflow geometry. We find in the simulations of the onset phase with narrow jets that a large fraction of the ejected mass outflows along the polar directions. The mass ejected at these directions has the fastest velocity and the highest angular momentum magnitude. In the simulations of the spiralling-in phase, a large fraction of the ejected mass concentrates around the orbital plane. According to our findings, the outflow with the highest velocity is closer to the poles as we launch narrower jets. The outflow has a toroidal shape accompanied by two faster rings, one ring at each side of the equatorial plane. The interaction of the jets with the giant envelope causes these outflow structures, as we do not include in our simulations the secondary star gravity and the envelope self-gravity." @default.
• W2890461387 created "2018-09-27" @default.
• W2890461387 creator A5008645637 @default.
• W2890461387 date "2018-09-06" @default.
• W2890461387 modified "2023-10-18" @default.
• W2890461387 title "The Morphology of the Outflow in the Grazing Envelope Evolution" @default.
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• W2890461387 doi "https://doi.org/10.3390/galaxies6030096" @default.
• W2890461387 hasPublicationYear "2018" @default.
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