No CrossRef data available.
Article contents
Combined Satellite and Ground-Based Observations of the Quiescent, High Latitude Symbiotic Variable AG Draconis = BD+67°922
Published online by Cambridge University Press: 12 April 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Satellite observations, from Einstein, IUE, and IRAS, have been combined with ground-based observations to derive the quiescent energy distribution of the symbiotic star AG Draconis. A detailed comparison is made between the combined observations and various steady-state composite models, including blackbody accretion disks.
- Type
- VII. Related Objects
- Information
- Copyright
- Copyright © Reidel 1987
References
Allen, D.A.
1979, in IAU Colloquium No. 46, ed. Bateson, F.M., Smak, J., and Uren, I.H. (New Zealand: University of Waikato), p. 125ff.Google Scholar
Blair, W.P., Stencel, R.E., Feibelman, W.A., and Michalitsianos, A.G.
1983, Astrophys. J. Suppl., 53, 573
CrossRefGoogle Scholar
Piro, L., Cassatella, A., Spinoglio, L., Viotti, R., and Altamore, A.
1985, IAU Circular No 4082.Google Scholar