Hostname: page-component-745bb68f8f-s22k5 Total loading time: 0 Render date: 2025-01-26T01:24:36.662Z Has data issue: false hasContentIssue false
  • English
  • Français

Analysis of the Balmer discontinuity behavior of Be stars by the Monte Carlo method

Published online by Cambridge University Press:  12 July 2011

Alicia Cruzado
Alicia Cruzado*
Affiliation:
Facultad de Ciencias Astrónomicas y Geofísicas, Universidad Nacional de La Plata, Paseo de Bosque s/n, La Plata, Buenos Aires, Argentina email: acruzado@fcaglp.unlp.edu.ar
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

For a given photospheric model, we study the behavior of the BD as different density and temperature distributions in the circumstellar envelope are assumed. For non spherically symmetric envelopes, we analyze the variation of the BD when the angle of observation varies. The radiation transfer through the medium is handled by means of the Monte Carlo method. We calculate the flux emitted by the star+envelope system in a small wavelength range around the BD. The calculations are made under LTE conditions.

Keywords

stars: early-typecircumstellar matter
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S272: Active OB stars: structure, evolution, mass loss, and critical limits , July 2010 , pp. 386 - 387
Copyright
Copyright © International Astronomical Union 2011

References

Crivellari, L. & Simonneau, E. 1994, ApJ 429, 331CrossRefGoogle Scholar
Gros, M., Crivellari, L. & Simonneau, E. 1997, ApJ 489, 331CrossRefGoogle Scholar
Zorec, J., Arias, M. L., Cidale, L., & Ringuelet, A. E. 2007, A&A 470, 239Google Scholar