No CrossRef data available.
Article contents
New Developments in Hot White Dwarf Models
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.
A short history of EUV observations of white dwarfs is presented, and how they have forced us to use increasingly sophisticated theoretical models—starting from blackbody spectra up to the present generation of NLTE models which include the blanketing effect of millions of atomic lines.
- Type
- IV. White Dwarf Structure/Evolution
- Information
- International Astronomical Union Colloquium , Volume 152: Astrophysics in the Extreme Ultraviolet , 1996 , pp. 185 - 192
- Copyright
- Copyright © Kluwer 1996
References
Kurucz, R.L.
1991, in Stellar Atmospheres: Beyond Classical Methods, ed. Crivellari, L.,, Hubeny, I. & Hummer, D.G., NATO ASI Ser. 341, 441
Google Scholar
Seaton, M.J., Zeippen, C.J., Tully, J.A.
et al.
1992, Rev. Mexicana Astron. Af., 23, 19
Google Scholar
Werner, K. & Dreizler, S.
1995, in Computational Astrophysics, II Stellar Physics, ed. Kndritzki, R.P., Mihalas, D., Nomoto, K., & Thielemann, F.-K., submittedGoogle Scholar
You have
Access