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The dynamics of a thin spherically-symmetric radiating shell

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Abstract

The conclusions of paper [2] are modified: using the shell formalism, relativistic effect could eventually be detected in X-ray bursters.

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Authors and Affiliations

  1. Instituto de Física Rosario (CONICET-UNR), Blvd. 27 de Febrero 210 bis, 2000, Rosario, Argentina

    Roberto O. Aquilano & Mario A. Castagnino

  2. Observatorio Astronómico Municipal de Rosario, Parque Urquiza, Casilla de Correo 606, 2000, Rosario, Argentina

    Roberto O. Aquilano, Mario A. Castagnino & Luis P. Lara

  3. Instituto de Astronomía y Física del Espacio, Casilla de Correo 67, Suc. 28, 1428, Buenos Aires, Argentina

    Mario A. Castagnino

  4. Facultad de Ciencias Exactas, Ingeniería y Agrimensura (UNR), Av. Pellegrini 250, 2000, Rosario, Argentina

    Luis P. Lara

Authors
  1. Roberto O. Aquilano
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  2. Mario A. Castagnino
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  3. Luis P. Lara
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Aquilano, R.O., Castagnino, M.A. & Lara, L.P. The dynamics of a thin spherically-symmetric radiating shell. Gen Relat Gravit 26, 525–530 (1994). https://doi.org/10.1007/BF02108053

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  • DOI: https://doi.org/10.1007/BF02108053

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