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V604 Aquilae or Nova Aquilae 1905 is a nova which was first observed in the constellation Aquila in 1905 with a maximum brightness of magnitude 7.6. It was never bright enough to be seen with the naked eye. It was discovered by Williamina Fleming on a Harvard College Observatory photographic plate taken on August 31, 1905. Examination of plates taken earlier indicates that peak brightness occurred in mid-August 1905. The star's quiescent visual band brightness is 19.6.

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  • V604 Aquilae (de)
  • V604 Aquilae (fr)
  • V604 Aquilae (en)
  • V604 Aquilae (sv)
  • 天鹰座V604 (zh)
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  • V604 Aquilae war eine Nova, die 1905 im Sternbild Adler erschien. Die Nova wurde am 31. August 1905 von W. Feming auf Fotoplatten der Harvard University entdeckt. Bei Durchsicht von älteren Fotoplatten ergab sich, dass die Nova Mitte August 1905 eine Maximalhelligkeit von 8,2 mag besaß. Im Jahre 1994 wurde eine Minimalhelligkeit von 19,6 mag gemessen. Weitere Messungen ergaben, dass die Helligkeit von V604 Aquilae unregelmäßig mit bis zu 0,25 mag variiert. (de)
  • V604 Aquilae (ou Nova Aquilae 1905) était une nova qui survint en 1905 dans la constellation de l'Aigle. Elle atteignit une magnitude minimale (correspondant à une luminosité maximale) de 7,6. (fr)
  • V604 Aquilae eller Nova Aquilae 1905 var en nova i stjärnbilden Örnen. Den upptäcktes den 14 augusti 1905 av Mrs W. Fleming som kring sekelskiftet upptäckte ett flertal novor. Som ljusstarkast blev novan magnitud +7,6. (sv)
  • 天鹰座V604(V604 Aquilae)也被称为1905年天鹰座新星(Nova Aquilae 1905)是一颗位于天鹰座的新星,1905年爆发。爆发时最亮视星等为7.6。 (zh)
  • V604 Aquilae or Nova Aquilae 1905 is a nova which was first observed in the constellation Aquila in 1905 with a maximum brightness of magnitude 7.6. It was never bright enough to be seen with the naked eye. It was discovered by Williamina Fleming on a Harvard College Observatory photographic plate taken on August 31, 1905. Examination of plates taken earlier indicates that peak brightness occurred in mid-August 1905. The star's quiescent visual band brightness is 19.6. (en)
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  • V604 Aquilae or Nova Aquilae 1905 (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/V604AqlLightCurve.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/V604AqlLocation.png
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  • V604 Aquilae war eine Nova, die 1905 im Sternbild Adler erschien. Die Nova wurde am 31. August 1905 von W. Feming auf Fotoplatten der Harvard University entdeckt. Bei Durchsicht von älteren Fotoplatten ergab sich, dass die Nova Mitte August 1905 eine Maximalhelligkeit von 8,2 mag besaß. Im Jahre 1994 wurde eine Minimalhelligkeit von 19,6 mag gemessen. Weitere Messungen ergaben, dass die Helligkeit von V604 Aquilae unregelmäßig mit bis zu 0,25 mag variiert. (de)
  • V604 Aquilae (ou Nova Aquilae 1905) était une nova qui survint en 1905 dans la constellation de l'Aigle. Elle atteignit une magnitude minimale (correspondant à une luminosité maximale) de 7,6. (fr)
  • V604 Aquilae or Nova Aquilae 1905 is a nova which was first observed in the constellation Aquila in 1905 with a maximum brightness of magnitude 7.6. It was never bright enough to be seen with the naked eye. It was discovered by Williamina Fleming on a Harvard College Observatory photographic plate taken on August 31, 1905. Examination of plates taken earlier indicates that peak brightness occurred in mid-August 1905. The star's quiescent visual band brightness is 19.6. V604 Aquilae faded by 3 magnitudes in just 25 days, making it a "fast nova". Detection of a faint nebula surrounding the star, with a radius of 0.4 arc minutes, was reported early in 1906. In 1994, a photometric study detected brightness variations of up to ~0.45 magnitudes on timescales of about one hour. An attempt to detect cool molecular gas surrounding the nova in 2015 was unsuccessful. (en)
  • V604 Aquilae eller Nova Aquilae 1905 var en nova i stjärnbilden Örnen. Den upptäcktes den 14 augusti 1905 av Mrs W. Fleming som kring sekelskiftet upptäckte ett flertal novor. Som ljusstarkast blev novan magnitud +7,6. (sv)
  • 天鹰座V604(V604 Aquilae)也被称为1905年天鹰座新星(Nova Aquilae 1905)是一颗位于天鹰座的新星,1905年爆发。爆发时最亮视星等为7.6。 (zh)
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