Talk:Supernova: Difference between revisions

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imported>Tomas Kindahl
imported>Johan Förberg
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==Split of from [[Nova (astronomy)]]==
==Split of from [[Nova (astronomy)]]==
Because currently considered unrelated to novae. Done today 19 July 2010. [[User:Tomas Kindahl|Tomas Kindahl]] 10:30, 19 July 2010 (UTC)
Because currently considered unrelated to novae. Done today 19 July 2010. [[User:Tomas Kindahl|Tomas Kindahl]] 10:30, 19 July 2010 (UTC)
== Diagram about nuclear binding energy ==
I added a diagram and chose to center it and interrupt the text flow. I think this is appropriate because the diagram is not a 'comment' but rather a vital part of the text. I realise that you may disagree, however. [[User:Johan A. Förberg|Johan A. Förberg]] 13:45, 19 July 2010 (UTC)

Revision as of 07:45, 19 July 2010

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 Definition:  An astronomical object exploding to a brightness similar to that of an entire galaxy. Caused by a catastrophic explosion of either a white dwarf system or an aged star about five times the size of the sun, which occurs when the star collapses; a neutron star or a black hole may be formed as a result, or the explosion results in no remaining compact object. [d] [e]
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Split of from Nova (astronomy)

Because currently considered unrelated to novae. Done today 19 July 2010. Tomas Kindahl 10:30, 19 July 2010 (UTC)

Diagram about nuclear binding energy

I added a diagram and chose to center it and interrupt the text flow. I think this is appropriate because the diagram is not a 'comment' but rather a vital part of the text. I realise that you may disagree, however. Johan A. Förberg 13:45, 19 July 2010 (UTC)

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