Bifurcations in thin spherically symmetric radiating shells
The conclusions of Ref. 1 are confirmed, using the shell formalism, relativistic effects could eventually be detected in X-ray bursters. We show in this letter that the oscillations could play an important role in the oscillation spectrum of these astronomical objects.
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| Otros Autores: | , |
| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
World Scientific Publishing Co. Pte Ltd
1996
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 03115caa a22004457a 4500 | ||
|---|---|---|---|
| 001 | PAPER-18936 | ||
| 003 | AR-BaUEN | ||
| 005 | 20241205090901.0 | ||
| 008 | 190411s1996 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-1542629725 | |
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| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Aquilano, R.O. | |
| 245 | 1 | 0 | |a Bifurcations in thin spherically symmetric radiating shells |
| 260 | |b World Scientific Publishing Co. Pte Ltd |c 1996 | ||
| 270 | 1 | 0 | |m Aquilano, R.O.; Instituto de Física Rosario, CONICET-UNR, Bv. 27 de Febrero 210 Bis, 2000 Rosario, Argentina |
| 504 | |a Aquilano, R., Castagnino, M., Lara, L., (1994) Gen. Rel. Grav., 26, p. 5 | ||
| 504 | |a Castagnino, M., Umérez, N., (1983) Gen. Rel. Grav., 15, p. 625 | ||
| 504 | |a Van den Heuvel, E.P.J., Rappaport, S.A., (1992) X-ray Binaries and Recycled Pulsars, , Kluwer | ||
| 504 | |a Hartle, J., (1973) Relativity, Astrophysics and Cosmology, , ed. W. Israel Reidel | ||
| 504 | |a Hamity, V., Gleiser, R., (1978) Astrophys. Space Sci., 58, p. 353 | ||
| 504 | |a Hamity, V., Spinosa, R., (1984) Gen. Rel. Grav., 16, p. 9 | ||
| 504 | |a Shore, S.N., Livio, M., Van den Heuvel, E.P.J., (1994) Observations and Physical Processes in Binary Stars, , Springer-Verlag | ||
| 504 | |a Lewin, W., Clark, G., (1980) Ann. N. Y. Acad. Sci., 336, p. 451 | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a The conclusions of Ref. 1 are confirmed, using the shell formalism, relativistic effects could eventually be detected in X-ray bursters. We show in this letter that the oscillations could play an important role in the oscillation spectrum of these astronomical objects. |l eng | |
| 593 | |a Fac. Cie. Exact., Ing. y Agrimensura, Universidad Nacional de Rosario, Av. Pellegrini 250, 2000 Rosario, Argentina | ||
| 593 | |a Instituto de Física Rosario, CONICET-UNR, Bv. 27 de Febrero 210 Bis, 2000 Rosario, Argentina | ||
| 593 | |a Inst. de Astronomia/Fis. del Espacio, CONICET-UBA, Casilla de Correos 67, Sucursal 28, 1428 Buenos Aires, Argentina | ||
| 593 | |a Observ. Astron./Planetario Munic., Parque Urquiza, Casilla de Correo 606, 2000 Rosario, Argentina | ||
| 700 | 1 | |a Castagnino, Mario Alberto | |
| 700 | 1 | |a Lara, L.P. | |
| 773 | 0 | |d World Scientific Publishing Co. Pte Ltd, 1996 |g v. 11 |h pp. 1115-1119 |k n. 14 |p Mod. Phys. Lett. A |x 02177323 |w (AR-BaUEN)CENRE-599 |t Modern Physics Letters A | |
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| 961 | |a paper_02177323_v11_n14_p1115_Aquilano |b paper |c PE | ||
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| 963 | |a VARI | ||