Advertisement

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
Chapter
  • 109 Downloads
Part of the Astrophysics and Space Science Library book series (ASSL, volume 233)

Abstract

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.

Keywords

Dust Emission Principal Quantum Number Dielectronic Recombination Stellar Radius Versus Filter 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  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

Personalised recommendations