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Spiral shock waves excited - PowerPoint PPT Presentation

Accretion onto Binary YSOs through Gap from Their Circumbinary Disk

Accretion onto Binary YSOs through Gap from Their Circumbinary Disk. Accretion rate of primary is larger than that of secondary. Accretion rate varies with a large amplitude. T. Hanawa, Y. Ochi, & K. Ando (Chiba Univ.). Majority of YSOs are multiple. UY Aur (Close et al. 1998). SPH model

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Spiral shock waves excited - PowerPoint PPT Presentation

Accretion onto Binary YSOs through Gap from Their Circumbinary Disk