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Paper: The Neon Abundance in WR Stars: Testing Massive Star Evolution
Volume: 388, Mass Loss from Stars and the Evolution of Stellar Clusters
Page: 233
Authors: Willis, A.J.; Crowther, P.; Morris, P.; van der Hucht, K.; Smith, J.D.T.; Marston, A.P.; Hillier, J.; Williams, P.
Abstract: The neon abundance in WR stars provides one of the most sensitive tests of massive star evolution theory being predicted to undergo enhancements of ×10 (WC phase) up to ×100 (WO phase). Results from ISO are summarized and our new IR programme with the Spitzer satellite is outlined.
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