论文信息 - Black hole transients and the Eddington limit - 字舞流文

Black hole transients and the Eddington limit

I show that the Eddington limit implies a critical orbital period P_crit(BH) = 2d beyond which black-hole LMXBs cannot appear as persistent systems. The unusual behaviour of GRO J1655-40 may result from its location close to this critical period.

A. R. King | A. King

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