PropertyValue
http://www.w3.org/1999/02/22-rdf-syntax-ns#type
http://www.w3.org/ns/prov#value
  • Another model for the formation of a Type Ia explosion involves the merger of two white dwarf stars, with the combined mass momentarily exceeding the Chandrasekhar limit.[47] A white dwarf could also accrete matter from other types of companions, including a main sequence star (if the orbit is sufficiently close).
http://www.w3.org/ns/prov#wasQuotedFrom
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