Publication Abstracts

Hartle et al. 1972

Hartle, J.B., K.S. Thorne, and S.M. Chitre, 1972: Slowly rotating relativistic stars. VI. Stability of the quasiradial modes. Astrophys. J., 176, 177-194, doi:10.1086/151620.

Equations are given for calculating the effects of a slow and rigid rotation on the frequency of the radial modes of oscillation of a relativistic star. The rotation is treated to second order in the angular velocity, but no other approximations are made.

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BibTeX Citation

@article{ha04410o,
  author={Hartle, J. B. and Thorne, K. S. and Chitre, S. M.},
  title={Slowly rotating relativistic stars. VI. Stability of the quasiradial modes},
  year={1972},
  journal={Astrophysical Journal},
  volume={176},
  pages={177--194},
  doi={10.1086/151620},
}

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RIS Citation

TY  - JOUR
ID  - ha04410o
AU  - Hartle, J. B.
AU  - Thorne, K. S.
AU  - Chitre, S. M.
PY  - 1972
TI  - Slowly rotating relativistic stars. VI. Stability of the quasiradial modes
JA  - Astrophys. J.
JO  - Astrophysical Journal
VL  - 176
SP  - 177
EP  - 194
DO  - 10.1086/151620
ER  -

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