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Eta Carinae: an Astrophysical Laboratory
Published online by Cambridge University Press: 09 August 2007
Abstract
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Eta Carinae (ηCar), a Luminous Blue Variable, is a massive binary star system with a 5.54-year spectroscopic period. We present temporal surface plots of selected He I, H I, Fe II and [N II] stellar line profiles measured with HST/STIS sampled from 1998.0 to 2004.3. Our analysis suggests that the profile variations are due to 1) radial velocity variations of the primary star and 2) ionization effects due to the hot companion combined with its wind cavity.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S240: Binary Stars as Critical Tools & Tests in Contemporary Astrophysics , August 2006 , pp. 666 - 669
- Copyright
- Copyright © International Astronomical Union 2007
References
Davidson, K., Smith, N., Gull, T.R., Ishibashi, K. & Hillier, D.J.
2001, AJ
121, 1569
CrossRefGoogle Scholar
Nielsen, K.E., Corcoran, M.F., Gull, T.R., Hillier, D.J., Hamaguchi, K., Ivarsson, S., & Lindler, D.J.
2006, ApJ submittedGoogle Scholar
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