B[e] Stars pp 131-133 | Cite as

Dielectronic Recombination of Mg II. Influence in the Infrared Continuum of B[e] Stars

  • Alicia Cruzado
  • Adela E. Ringuelet
  • Héctor O. Di Rocco
Part of the Astrophysics and Space Science Library book series (ASSL, volume 233)


We investigated the dielectronic recombination of MgII in low density and low temperature media; we concluded that it may contribute to the IR excess in Be stars.


Dust Emission Principal Quantum Number Dielectronic Recombination Stellar Radius Versus Filter 
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  1. Allen, D. A. 1973, Mon. Not. R. astr. Soc., 161, 145ADSGoogle Scholar
  2. Gehrz, R. D., Hackwell, J. A., Jones, T. W. 1974, ApJ, 191, 675ADSCrossRefGoogle Scholar
  3. Vazquez, A. C., Cidale, L. S., Ringuelet A. E. 1993, 419, 286Google Scholar
  4. Waters, L. B. F. M. 1986, A&A, 162, 121ADSGoogle Scholar
  5. Waters, L. B. F. M., Coté, J., Lamers, H. J. G. L. M. 1987, 185, 206Google Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1998

Authors and Affiliations

  • Alicia Cruzado
    • 1
  • Adela E. Ringuelet
    • 1
  • Héctor O. Di Rocco
    • 2
  1. 1.Observatorio Astronómico de La PlataLa PlataArgentina
  2. 2.Instituto de Física de Arroyo SecoTandilArgentina

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