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- | title=Ozone Depletion from Nearby Supernovae ...olution of main sequence star + white dwarf binary systems towards Type Ia supernovae ...42 KB (6,228 words) - 21:20, 5 February 2010
- ...277..791N Evolution of 8–10 solar mass stars toward electron capture supernovae. I - Formation of electron-degenerate O + Ne + Mg cores], Ken'ichi Nomoto, ===Type Ia supernovae=== ...77 KB (11,681 words) - 21:21, 5 February 2010
- | title = The Historical Supernovae | booktitle = Supernovae: A survey of current research; Proceedings of the Advanced Study Institute ...96 KB (14,170 words) - 15:20, 20 August 2009
- ...these regions to collapse. Because only massive, short-lived stars produce supernovae, the Sun must have formed in a large star-forming region which produced mas ...s, which live for relatively short periods and then explode violently as [[supernovae]].<ref>{{cite journal|title=Mass Extinctions and The Sun's Encounters with ...85 KB (12,829 words) - 17:09, 18 August 2009
- 71 KB (10,454 words) - 13:19, 15 March 2011
- ...r System's current location, some scientists have hypothesised that recent supernovae may have adversely affected life in the last 35,000 years by flinging piece ...high-temperature plasma that suggests it is the product of several recent supernovae.<ref>{{cite web |title=Near-Earth Supernovas |work=NASA |url=http://science ...82 KB (12,278 words) - 17:12, 18 August 2009
- ...theories are unable to account for timescale stretch observed in [[type Ia supernovae]]</ref> ...66 KB (9,812 words) - 01:07, 12 August 2009
- | title=Supernovae and Nucleosynthesis: An Investigation of the History of Matter, from the Bi ...49 KB (7,190 words) - 18:56, 4 June 2009
- ...or, for more recent numerical work, {{Harvnb|Font|2003|loc=sec. 4.1}}; for supernovae, there are still major problems to be solved, cf. {{Harvnb|Buras|Rampp|Jank ...160 KB (21,329 words) - 06:49, 19 August 2009
- 94 KB (13,468 words) - 17:06, 20 August 2009