Binary evolution with relativistic jets

Details Binary evolution with relativistic jets Binary evolution with relativistic jets

1998-10-20

arxiv.org/abs/astro-ph/9810317v1

New Astron.Rev. 42 (1998) 609-612

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures; to appear in 2nd Workshop of Relativistic Jets from Galactic Sources, R.N.Ogley and S.J.Bell Burnell (eds.

Scientific paper

10.1016/S1387-6473(98)00082-7

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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