Anisotropic mass ejection in binary mergers

Anisotropic mass ejection in binary mergers

We investigate the mass loss from a rotationally distorted envelope following the early, rapid in-spiral of a companion star inside a common envelope. For initially wide, massive binaries (M_1+M_2=20M_{\odot}, P\sim 10 yr), the primary has a convective envelope at the onset of mass transfer and is a...

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Dettagli Bibliografici
Autori principali:	Morris, T, Podsiadlowski, P
Natura:	Journal article
Pubblicazione:	2005

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