What is it about?
G35-26 is the name of a type of stars known as WhiteDwarf stars. This particular WD appeared to have a very large mass for irs type.
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Why is it important?
Its large mass was a challenge for theories of how stars evole.
Perspectives
Later, someone else obtained better spectroscopic data and was able to show that the star was more normal than we thought.
Doc Peter Thejll
Danish Meteorological INstitute
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This page is a summary of: The DBAQ G35–26, January 1991, Springer Science + Business Media,
DOI: 10.1007/978-94-011-3230-5_29.
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