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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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