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Unstable mass transfer - PowerPoint PPT Presentation

Using Observables in LMXBs to Constrain the Nature of Pulsar

Using Observables in LMXBs to Constrain the Nature of Pulsar. Dong, Zhe & Xu, Ren-Xin Peking University Sep. 16 th 2006. Outline. Motivation Phenomena Predicting after Releasing the Mass-Constraint upon Pulsar Discussion upon Accretion Phenomenon Conclusion and Prospect. Outline.

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Binary Star Evolution

Binary Star Evolution. Half of all stars are in binary systems - stellar evolution in binaries is important Roche Lobe: 3-D boundary where the gravity of 2 stars is equal; if a star expands beyond this boundary some of its matter accretes onto the other star

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1.21k views • 24 slides

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Unstable mass transfer - PowerPoint PPT Presentation

Using Observables in LMXBs to Constrain the Nature of Pulsar

Binary Star Evolution