| Autor: |
Collins, G. W., Foltz, C. B. |
| Zdroj: |
Publications of the Astronomical Society of the Pacific; December 1977, Vol. 89 Issue: 532 p896-896, 1p |
| Abstrakt: |
A new mechanism for the origin of the nova outburst is presented. A magnetic white dwarf in a binary system undergoes collapse. This collapse induces pressure disturbance which propagates along the field lines, expelling the polar regions of the star. It is found that the energy of the outburst depends on the magnetic field of the configuration. Key words: novae-white dwarfs-stellar interiors |
| Databáze: |
Supplemental Index |
| Externí odkaz: |
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