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Spectrum Analysis of the Cool White Dwarfs G 128-7 and G 165-7
Published online by Cambridge University Press: 12 April 2016
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The cool white dwarf stars G 128-7 and G 165-7 have a quite different character: While the line spectrum of G 165-7 is the richest of all white dwarfs known, G 128-7 shows only a strong Hα line (Wλ ≈ 5.5 Å) and a much weaker Hβ line (Wλ ≈ 1 Å).
- Type
- Colloquium Session III
- Information
- International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 184 - 185
- Copyright
- Copyright © The University of Rochester 1979
References
Liebert, J., Angel, J. R. P. and Landstreet, J. D.
1975
Ap. J. (Letters)
202, L139.CrossRefGoogle Scholar
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