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- CE_Gruis abstract "CE Gruis is a (also known as Grus V-1) is a faint (magnitude 18–21) binary star system in the constellation Grus. It is composed of a white dwarf and donor star, in this case the two are so close and fused into orbit facing one another. Known as polars, material from the donor star does not form an accretion disc around the white dwarf, but rather streams directly onto it.".
- CE_Gruis wikiPageID "41896644".
- CE_Gruis wikiPageRevisionID "594849136".
- CE_Gruis constell Grus_(constellation).
- CE_Gruis name "CE Gruis".
- CE_Gruis subject Category:Binary_stars.
- CE_Gruis subject Category:Grus_(constellation).
- CE_Gruis subject Category:Objects_named_with_variable_star_designations.
- CE_Gruis subject Category:Polars_(cataclysmic_variable_stars).
- CE_Gruis comment "CE Gruis is a (also known as Grus V-1) is a faint (magnitude 18–21) binary star system in the constellation Grus. It is composed of a white dwarf and donor star, in this case the two are so close and fused into orbit facing one another. Known as polars, material from the donor star does not form an accretion disc around the white dwarf, but rather streams directly onto it.".
- CE_Gruis label "CE Gruis".
- CE_Gruis sameAs m.0_qlqg4.
- CE_Gruis sameAs Q17006858.
- CE_Gruis sameAs Q17006858.
- CE_Gruis wasDerivedFrom CE_Gruis?oldid=594849136.
- CE_Gruis isPrimaryTopicOf CE_Gruis.