ISO spectroscopy of Luminous Blue Variables as a probe of post main sequence massive star evolution

Details ISO spectroscopy of Luminous Blue Variables as a probe of post main sequence massive star evolution ISO spectroscopy of Luminous Blue Variables as a probe of post main sequence massive star evolution

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000esasp.456..165m&link_type=abstract

ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy. Eds. A. Salama, M.F.Kessler, K. Leech & B. Schulz. ESA-SP

Physics

Iso

Scientific paper

IR spectroscopy of dust in the nebula surrounding hot, massive stars is
a useful probe of the evolutionary state of the stellar source at the
time of dust production. We review the latest results of ISO
spectroscopic studies of the dust in nebulae of Luminous Blue Variable
(LBV) stars AG Carinae, η Carinae, and LBV-candidate Wra 751.

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