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Bozzo, E., Stella, L., Vietri, M., Ghosh, P. (2009) Can disk-magnetosphere interaction models and beat frequency models for quasi-periodic oscillation in accreting X-ray pulsars be reconciled?. Astronomy & Astrophysics, 493 (3). 809-818 doi:10.1051/0004-6361:200810658

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Reference TypeJournal (article/letter/editorial)
TitleCan disk-magnetosphere interaction models and beat frequency models for quasi-periodic oscillation in accreting X-ray pulsars be reconciled?
JournalAstronomy & Astrophysics
AuthorsBozzo, E.Author
Stella, L.Author
Vietri, M.Author
Ghosh, P.Author
Year2009 (January)Volume493
Issue3
PublisherEDP Sciences
DOIdoi:10.1051/0004-6361:200810658Search in ResearchGate
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Mindat Ref. ID3471985Long-form Identifiermindat:1:5:3471985:1
GUID0
Full ReferenceBozzo, E., Stella, L., Vietri, M., Ghosh, P. (2009) Can disk-magnetosphere interaction models and beat frequency models for quasi-periodic oscillation in accreting X-ray pulsars be reconciled?. Astronomy & Astrophysics, 493 (3). 809-818 doi:10.1051/0004-6361:200810658
Plain TextBozzo, E., Stella, L., Vietri, M., Ghosh, P. (2009) Can disk-magnetosphere interaction models and beat frequency models for quasi-periodic oscillation in accreting X-ray pulsars be reconciled?. Astronomy & Astrophysics, 493 (3). 809-818 doi:10.1051/0004-6361:200810658
In(2009, January) Astronomy & Astrophysics Vol. 493 (3) EDP Sciences

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