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Spectral Analysis of the LMC [WC] Star SMP 61

  • G. Gräfener (a1), W.-R. Hamann (a1) and M. Peña (a2)

Abstract

HST UV and optical spectra of the early-type [WC] star SMP 61 in the LMC are analyzed by means of line blanketed non-LTE models for expanding atmospheres. The known distance to the LMC allows a reliable determination of the stellar parameters. The low iron surface abundance of the object possibly indicates a preceding evolution through a very late thermal pulse (VLTP).

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References

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Gräfener, G., Koesterke, L., Hamann, W.-R. 2002, submitted to A&A
Hillier, D. J., & Miller, D. L. 1999, ApJ 519, 354
Peña, M., Ruiz, M. T., Torres-Peimbert, S. 1997, A&A 324, 674

Spectral Analysis of the LMC [WC] Star SMP 61

  • G. Gräfener (a1), W.-R. Hamann (a1) and M. Peña (a2)

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