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- Q6458 subject Q7061010.
- Q6458 subject Q8880743.
- Q6458 abstract "Template:ForA nova (plural novae or novas) is a cataclysmic nuclear explosion on a white dwarf, which causes a sudden brightening of the star. Novae are not to be confused with other brightening phenomena such as supernovae or luminous red novae. Novae are thought to occur on the surface of a white dwarf in a binary system when they are sufficiently near to one another, allowing material (mostly hydrogen) to be pulled from the companion star's surface onto the white dwarf. The nova is the result of the rapid fusion of the accreted hydrogen on the surface of the star, commencing a runaway fusion reaction.".
- Q6458 thumbnail Making_a_Nova.jpg?width=300.
- Q6458 wikiPageExternalLink 0501.shtml.
- Q6458 wikiPageExternalLink novae.html.
- Q6458 wikiPageExternalLink gcvs.
- Q6458 wikiPageWikiLink Q10464.
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- Q6458 wikiPageWikiLink Q7061010.
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- Q6458 wikiPageWikiLink Q8880743.
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- Q6458 type Thing.
- Q6458 comment "Template:ForA nova (plural novae or novas) is a cataclysmic nuclear explosion on a white dwarf, which causes a sudden brightening of the star. Novae are not to be confused with other brightening phenomena such as supernovae or luminous red novae. Novae are thought to occur on the surface of a white dwarf in a binary system when they are sufficiently near to one another, allowing material (mostly hydrogen) to be pulled from the companion star's surface onto the white dwarf.".
- Q6458 label "Nova".
- Q6458 depiction Making_a_Nova.jpg.