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QU Vulpeculae, also known as Nova Vulpeculae 1984 Number 2, was the second nova which occurred in 1984 in the constellation Vulpecula ( was the first). It was discovered by Peter Collins, an amateur astronomer from Cardiff, California at 22:08 UT on 22 December 1984. At the time of its discovery, the nova's apparent magnitude was 6.8. By the next night, Collins reported its brightness had increased to magnitude 5.6, making it visible to the naked eye. QU Vulpeculae declined from peak brightness quite rapidly, and had faded by 3 magnitudes in just 40 days, so it is classified as a "fast" nova.

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  • QU Vulpeculae (de)
  • QU Vulpeculae (eu)
  • QU Vulpeculae (es)
  • QU Vulpeculae (fr)
  • QU Vulpeculae (en)
  • QU Vulpeculae (sv)
  • 狐狸座QU (zh)
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  • QU Vulpeculae war eine Nova, die 1984 im Sternbild Fuchs aufleuchtete und die eine Helligkeit von 5,2 mag erreichte. Der Namensteil „QU“ folgt den Regeln zur Benennung veränderlicher Sterne und besagt, dass QU Vulpeculae der 329. veränderliche Stern ist, der im Sternbild Fuchs entdeckt wurde. (de)
  • QU Vulpeculae Vulpecula konstelazioan agertutako noba bat da. 1984. urtean deskubritu zen. Noba horrek 5.2 magnitudeko distira lortu zuen. (eu)
  • QU Vulpeculae (ou Nova Vulpeculae 1984 b) était une nova qui survint en 1984 dans la constellation du Petit Renard. Elle atteignit une magnitude minimale (correspondant à une luminosité maximale) de 5,2. (fr)
  • En astronomía, QU Vulpeculae es el nombre que los astrónomos le dieron a la nova aparecida en la constelación de Vulpecula,​ en el año 1984, la cual alcanzó un brillo de magnitud 5.2.​ (es)
  • QU Vulpeculae var en nova som upptäcktes den 25 december 1984 i stjärnbilden Räven, som i maximum nådde +5,2 i magnitud. QU Vulpeculae klassificeras som neonnova, eller ONeMg. Den är en kataklysmisk variabel av typen AM Herculis med omloppstiden 2,6 timmar. (sv)
  • 狐狸座QU(QU Vulpeculae)是一颗位于狐狸座的新星,1984年爆发。爆发时最亮视星等为5.2。 (zh)
  • QU Vulpeculae, also known as Nova Vulpeculae 1984 Number 2, was the second nova which occurred in 1984 in the constellation Vulpecula ( was the first). It was discovered by Peter Collins, an amateur astronomer from Cardiff, California at 22:08 UT on 22 December 1984. At the time of its discovery, the nova's apparent magnitude was 6.8. By the next night, Collins reported its brightness had increased to magnitude 5.6, making it visible to the naked eye. QU Vulpeculae declined from peak brightness quite rapidly, and had faded by 3 magnitudes in just 40 days, so it is classified as a "fast" nova. (en)
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  • QU Vulpeculae (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/QUVulLightCurve.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/QUVulLocation.png
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  • QU Vulpeculae war eine Nova, die 1984 im Sternbild Fuchs aufleuchtete und die eine Helligkeit von 5,2 mag erreichte. Der Namensteil „QU“ folgt den Regeln zur Benennung veränderlicher Sterne und besagt, dass QU Vulpeculae der 329. veränderliche Stern ist, der im Sternbild Fuchs entdeckt wurde. (de)
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