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An exact, three-dimensional, time-dependent wave solution in local Keplerian flow

Publication status:: Published

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APA Style

Balbus, S., & Hawley, J. (2006). An exact, three-dimensional, time-dependent wave solution in local Keplerian flow. ASTROPHYSICAL JOURNAL, 652(2), 1020–1027.

MLA Style

Balbus, S, and J Hawley. “An Exact, Three-Dimensional, Time-Dependent Wave Solution in Local Keplerian Flow.” ASTROPHYSICAL JOURNAL, vol. 652, no. 2, 2006, pp. 1020–27.

Chicago Style

Balbus, S, and J Hawley. 2006. “An Exact, Three-Dimensional, Time-Dependent Wave Solution in Local Keplerian Flow.” ASTROPHYSICAL JOURNAL 652 (2): 1020–27.
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Publisher copy:: 10.1086/508320

Authors

+ Balbus, S More by this author

Institution:: University of Oxford
Division:: MPLS
Department:: Physics
Sub department:: Astrophysics
Role:: Author

+ Hawley, J More by this author

Role:: Author

Journal:: ASTROPHYSICAL JOURNAL More from this journal
Volume:: 652
Issue:: 2
Pages:: 1020-1027
Publication date:: 2006-12-01
DOI:: 10.1086/508320
EISSN:: 1538-4357
ISSN:: 0004-637X

Keywords:: galaxies : magnetic fields

MHD

accretion, accretion disks

magnetic fields

instabilities
Pubs id:: pubs:333932
UUID:: uuid:e8ccd0bd-3524-40cd-8ffd-38b95eb01673
Local pid:: pubs:333932
Source identifiers:: 333932
Deposit date:: 2015-01-13
ARK identifier:: ark:/29072/ora_e8ccd0bd352440cd8ffd38b95eb01673

Terms of use

Copyright date:: 2006

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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