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.
- Get PDF (1.6 MB. Document is scanned, no OCR.)
- PDF documents require the free Adobe Reader or compatible viewing software to be viewed.
- Go to journal article webpage
Export citation: [ BibTeX ] [ RIS ]
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}, }
[ Close ]
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 -
[ Close ]