Can disk-magnetosphere interaction models and beat frequency models for quasi-periodic oscillation in accreting X-ray pulsars be reconciled?

Publisher： Edp Sciences

E-ISSN： 1432-0746|493|3|809-818

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.493, Iss.3, 2009-01, pp. : 809-818

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