Common Envelope Binaries and Mass Loss
In this work we calculate the evolution of a binary system with a common envelope, which consists of a blue supergiant and a neutron star. We consider as a free parameter the effectivity with which the energy liberated at the orbit produces mass loss from the system.
The evolutionary calculations were made, using various values of this parameter, for a system with mass ratio 25:1. As initial state we choose a model in the phase of Hydrogen-shell burning, before and after the begin of Helium-burning in the core.
We found that, under certain conditions, it is possible for the radius of the orbit and the period of the system to increase; the time scale for the “spiral-in” would be of the order of 104–105 years. Mass loss rates are between 10−3 M☉/y and 10−4 M☉/y.
KeywordsNeutron Star Mass Loss Rate Mass Accretion Rate Common Envelope Helium Star
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