PG1159-035
1. PG 1159-035PG 1159-035 is the prototypical PG 1159 star after which the class of PG 1159 stars was named. It was discovered in the Palomar-Green survey of ultraviolet-excess stellar objects and, like the other PG 1159 stars, is in transition between being the central star of a planetary nebula and being a white dwarf. The luminosity of PG 1159-035 was observed to vary in 1979, and it was given the variable star designation GW Vir in 1985.
Read “PG 1159-035” on English Wikipedia
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Read “PG 1159-035” on DBpedia
Read “PG 1159-035” on English Wikipedia
Read “PG1159-035” on Japanese Wikipedia
Read “PG 1159-035” on DBpedia
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