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Binary evolution with relativistic jets

Ulrich Kolb
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Abstract

Relativistic jets can extract mass-energy from a black hole. In semi-detached black hole binaries the jet ejection process constitutes a `consequential angular momentum loss' (CAML) process. The effect of this jet-induced CAML is to lower the transfer rate below the value set by systemic driving and to stabilize otherwise unstable systems. Implications of jet-induced CAML for GRO J1655-40 are discussed.

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Ulrich Kolb. 1998-10-20. Binary evolution with relativistic jets. https://doi.org/10.1016/s1387-6473(98)00082-7

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