Nonlinear development of the secular bar-mode instability in rotating neutron stars
- Author
- SHANGLI OU1 ; TOHLINE, Joel E1 ; LINDBLOM, Lee2
[1] Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA 70803, United States
[2] Theoretical Astrophysics, MS 130-33, California Institute of Technology, Pasadena, CA 91125, United States - Source
The Astrophysical journal. 2004, Vol 617, Num 1, pp 490-499, 10 p ; 1 ; ref : 76 ref
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- University of Chicago Press, Chicago, IL
- Publication country
- United States
- Document type
- Article
- Language
- English
- Keyword (fr)
- Etoile neutron Instabilité séculaire Modèle hydrodynamique Onde gravitationnelle
- Keyword (en)
- Neutron stars Secular instability Hydrodynamic model Gravitational waves
- Keyword (es)
- Inestabilidad secular
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C60 Late stages of stellar evolution (including black holes) / 001E03C60J Neutron stars
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 16387311
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1086/425296 
https://dx.doi.org/10.1086/425296
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