Advertisement

B[e] Stars pp 227-228 | Cite as

Infrared Emission from Dust around B[e] Stars

  • Ivezić Željko
  • Anatoly S. Miroshnichenko
  • Elitzur Moshe
Chapter
  • 113 Downloads
Part of the Astrophysics and Space Science Library book series (ASSL, volume 233)

Abstract

Many B[e] stars show IR excess indicating the presence of circumstellar dust. However, HD 45677 is the only such star with a detailed model of its spectral energy distribution (SED), computed by Sorrell (1989). Here we present such modeling in the wavelength range 0.3 – 100 μm for a sample of 13 B[e] stars.

Keywords

Spectral Type Spectral Energy Distribution Infrared Emission Interstellar Dust Interstellar Extinction 
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.

References

  1. Draine, B.T., Lee, H.M, 1984, ApJ, 285, 89ADSCrossRefGoogle Scholar
  2. Ivezic, Z., Nenkova, M., & Elitzur, M.: 1997, Univ. of Kentucky, Internal ReportGoogle Scholar
  3. Kurucz, R.L. 1979, ApJS, 40, 1ADSCrossRefGoogle Scholar
  4. Sorrell, W.H. 1989. MNRAS, 241, 89ADSGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1998

Authors and Affiliations

  • Ivezić Željko
    • 1
  • Anatoly S. Miroshnichenko
    • 2
  • Elitzur Moshe
    • 3
  1. 1.Department of Astrophysical SciencesPrinceton UniversityPrincetonUSA
  2. 2.Central Astronomical Observatory of the Russian Academy of Sciences at PulkovoSaint-PetersburgRussia
  3. 3.Department of Physics and AstronomyUniversity of KentuckyLexingtonUSA

Personalised recommendations