Wide binaries - PowerPoint PPT Presentation

Julio Chanam é

Wide Binaries: the non-violent end of the semi-major axis distribution. Julio Chanam é. Hubble Fellows Symposium 2010. Wide Binaries: the non-violent end of the semi-major axis distribution. Julio Chanam é. Hubble Fellows Symposium 2010. Massive Black Holes and Stellar Dynamics in

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663 views • 54 slides

Getting to Eddington and beyond in AGN and binaries!

Getting to Eddington and beyond in AGN and binaries!. Chris Done University of Durham. Accreting black holes. L / L Edd determined by mass accretion rate onto the black hole LMXRB – roche lobe overflow of low mass companion HMXRB – wind accretion from high mass companion

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NA Kaib et al. Nature 000 , 1-4 (2012) doi:10.1038/nature11780

Eccentricity excitation of planets of wide binaries. NA Kaib et al. Nature 000 , 1-4 (2012) doi:10.1038/nature11780.

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