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U Aquarii, abbreviated U Aqr, is a variable star in the equatorial constellation of Aquarius. It is invisible to the naked eye, having an apparent visual magnitude that ranges from 10.6 down to as low as 15.9. Based on parallax measurements, the distance to this star is approximately 38 kly (12 kpc). In 1990, W. A. Lawson and associates provided a distance estimate of 43 kly (13.2 kpc) based on the assumption of a bolometric magnitude of −5. It appears to lie several kiloparsecs below the galactic plane, and thus may belong to an old stellar population.

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rdf:type
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  • U Aquarii (fr)
  • みずがめ座U星 (ja)
  • U Aquarii (pl)
  • U Водолея (ru)
  • U Aquarii (en)
  • U Aquarii (sv)
  • 寶瓶座U (zh)
rdfs:comment
  • U Aquarii (U Aqr) est une étoile de la constellation du Verseau. Il s'agit d'une étoile variable de type R Coronae Borealis dont la magnitude apparente varie entre 10,6 et 15,9. En 1999, il a été proposé que U Aqr soit un objet de Thorne-Zytkow, plutôt qu'une simple variable de type R Coronae Borealis. (fr)
  • U Aquarii – gwiazda zmienna typu R Coronae Borealis położona w gwiazdozbiorze Wodnika. Według niektórych hipotez gwiazda jest obiektem Thorne-Żytkow, olbrzymem z gwiazdą neutronową w jądrze. (pl)
  • U Aquarii är en eruptiv variabel av RCB-typ (RCB) i stjärnbilden Vattumannen. Stjärnan har magnitud +10,8 och når i förmörkelsefasen ner till +18,2. (sv)
  • 寶瓶座U(U Aquarii、U Aqr)是位於寶瓶座的一顆恆星,屬於北冕座R型變星。該恆星的視星等在10.6到15.9之間變化。有觀測證據顯示寶瓶座U可能是尚未被證實存在的索恩-祖特阔夫天体。 (zh)
  • U Водолея (лат. U Aquarii) — одиночная переменная звезда в созвездии Водолея на расстоянии (вычисленном из значения параллакса) приблизительно 17112 световых лет (около 5247 парсеков) от Солнца. Видимая звёздная величина звезды — от +15,9m до +10,6m. (ru)
  • U Aquarii, abbreviated U Aqr, is a variable star in the equatorial constellation of Aquarius. It is invisible to the naked eye, having an apparent visual magnitude that ranges from 10.6 down to as low as 15.9. Based on parallax measurements, the distance to this star is approximately 38 kly (12 kpc). In 1990, W. A. Lawson and associates provided a distance estimate of 43 kly (13.2 kpc) based on the assumption of a bolometric magnitude of −5. It appears to lie several kiloparsecs below the galactic plane, and thus may belong to an old stellar population. (en)
  • みずがめ座U星 (U Aquarii, U Aqr) は、みずがめ座の領域にある恒星で、かんむり座R型変光星に分類される変光星。恒星大気中の炭素の存在量が酸素よりも多い炭素星で、その中でも、水素吸収線がほとんど見られない「水素欠乏型炭素星 (HdC, hydrogen deficient carbon star) 」に分類される。太陽系からの距離は、ガイア計画の第2回データリリースの年周視差からは17,000光年、第3回初期データリリースからは38,000光年と、未だ十分に定まっていない。 (ja)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/UAqrLightCurve.png
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  • C-Hd (en)
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