NLTE Analysis of R84

  • W. Schmutz
  • C. Leitherer
  • A. V. Torres-Dodgen
  • M. Vogel
  • P. S. Conti
  • W.-R. Hamann
  • U. Wessolowski
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 157)

Abstract

The LMC star R84 (-HDE 269227 -BR 18) belongs to the group of Ofpe/WN stars believed to be closely related to the Luminous Blue Variables. Support for such a relation comes from the spectral resemblance of these stars to AG Car during visual minimum, and from the observed outburst of the Ofpe/WN star R127.

Keywords

Helium Abundance Continuum Flux Free Model Parameter Laboratory Astrophysics Stellar Temperature 
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. Maeder,A., Meynet,G.:1987, Astron. Astrophys. 182, 243Google Scholar
  2. Stahl,0., Wolf,B., de Groot,M., Leitherer,C.: 1985, Astron. Astrophys. Suppl. 61, 237Google Scholar
  3. Wessolowski, U., Schmutz, W., Hamann,W.-R.: 1988, A. & A. 194, 160ADSGoogle Scholar

Copyright information

© Kluwer Academic Publishers 1989

Authors and Affiliations

  • W. Schmutz
    • 1
  • C. Leitherer
    • 1
  • A. V. Torres-Dodgen
    • 1
  • M. Vogel
    • 2
  • P. S. Conti
    • 1
  • W.-R. Hamann
    • 3
  • U. Wessolowski
    • 3
  1. 1.Joint Institute for Laboratory AstrophysicsUniversity of Colorado and National Bureau of StandardsBoulderUSA
  2. 2.Institut für AstronomieETH ZentrumZurichSwitzerland
  3. 3.Institut für Theoretische Physik und SternwarteUniversität KielKielGermany

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