Document Type
Article
Publication Date
4-1-2006
Abstract
We have obtained new optical spectra with the ESO/VLT of the final helium flash star, V605 Aql. These spectra, indicate that V605 Aql has evolved significantly in only 80 years. It now has a T eff ∼95,000 K and has abundances similar to those seen in [WC] central stars but not to those of a typical RCB star. © 2006 International Astronomical Union.
Publication Source (Journal or Book title)
Proceedings of the International Astronomical Union
First Page
379
Last Page
380
Recommended Citation
Clayton, G., Fedrow, J., Crowther, P., Kerber, F., Pirzkal, N., & De Marco, O. (2006). V605 Aql: 80 years after the final helium shell flash. Proceedings of the International Astronomical Union, 2 (234), 379-380. https://doi.org/10.1017/S1743921306003334
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