W Cygni
http://dbpedia.org/resource/W_Cygni an entity of type: Thing
はくちょう座W星（はくちょうざダブリューせい）は、はくちょう座にある有名な半規則型変光星のことである。学名はW Cygni（略称はW Cyg）で、典型的な赤色巨星である。
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W Cygni är en halvregelbunden variabel av SRB-typ i stjärnbilden Svanen. Stjärnan varierar mellan magnitud +5,10 och 6,83 med en period av 131,7 dygn. Den har en sekundär period som uppmätts till 235,3 dygn (GCVS) och 260 dygn (Otero).
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天鵝座W，又名BD+44 3877，HD 205730、SAO 51079、HR 8262，是天鵝座的一颗恒星，视星等为5.53，位于銀經90.86，銀緯-4.98，其B1900.0坐标为赤經21h 32m 14.3s，赤緯+44° -4.98′ 36″。
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W Cygni is a semi-regular variable star in the constellation Cygnus, located 570 light-years from Earth. It lies less than half a degree southeast of ρ Cygni. W Cygni is, at times, a naked-eye star but it was not given a Bayer or Flamsteed designation. It has been proposed as a binary star system with a hotter main sequence companion, but this has not been confirmed.
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はくちょう座W星
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W Cygni
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W Cygni
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天鵝座W
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W Cygni
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M4e-M6eIII
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W Cygni is a semi-regular variable star in the constellation Cygnus, located 570 light-years from Earth. It lies less than half a degree southeast of ρ Cygni. W Cygni is, at times, a naked-eye star but it was not given a Bayer or Flamsteed designation. It has been proposed as a binary star system with a hotter main sequence companion, but this has not been confirmed. W Cygni was discovered to be variable by John Ellard Gore, and first published in 1885. It has a maximum magnitude of 5.10 and a minimum magnitude 6.83. The star is catalogued as having a primary period of 131.7 days, but shows variations with a variety of periods around 131 days as well as 234 days. It is believed to be pulsating in the first overtone. There is some evidence of additional very slow and small variations in the light curve on a time scale of 3,000–5,000 days. This star is an aging red giant on the asymptotic giant branch (AGB). Its spectral type ranges between M4e and M6e, and it shows possible elevated levels of Technetium. The masses of AGB stars are poorly known, but using the pulsation properties of W Cygni, it mass is calculated to be slightly less than the sun's. It has expanded to 227 times the girth of the Sun and is radiating 5,888 times the Sun's luminosity from its swollen photosphere at an effective temperature of 3,373 K.
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はくちょう座W星（はくちょうざダブリューせい）は、はくちょう座にある有名な半規則型変光星のことである。学名はW Cygni（略称はW Cyg）で、典型的な赤色巨星である。
rdf:langString
W Cygni är en halvregelbunden variabel av SRB-typ i stjärnbilden Svanen. Stjärnan varierar mellan magnitud +5,10 och 6,83 med en period av 131,7 dygn. Den har en sekundär period som uppmätts till 235,3 dygn (GCVS) och 260 dygn (Otero).
rdf:langString
天鵝座W，又名BD+44 3877，HD 205730、SAO 51079、HR 8262，是天鵝座的一颗恒星，视星等为5.53，位于銀經90.86，銀緯-4.98，其B1900.0坐标为赤經21h 32m 14.3s，赤緯+44° -4.98′ 36″。
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7742
