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NGC 3603-C (HD 97950C) is a single-lined spectroscopic binary star system located at the centre of the HD 97950 cluster in the NGC 3603 star-forming region, about 25,000 light years from Earth. The primary has spectral type WN6h and is among the most luminous and most massive known. HD 97950 was catalogued as a star, but was known to be a dense cluster or close multiple star. In 1926, the six brightest members were given letters from A to F, although several of them have since been resolved into more than one star. Star C was shown to be a binary, but its companion has not been observed.

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  • NGC 3603-C (en)
  • NGC 3603-C (ru)
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  • NGC 3603-C (HD 97950C) is a single-lined spectroscopic binary star system located at the centre of the HD 97950 cluster in the NGC 3603 star-forming region, about 25,000 light years from Earth. The primary has spectral type WN6h and is among the most luminous and most massive known. HD 97950 was catalogued as a star, but was known to be a dense cluster or close multiple star. In 1926, the six brightest members were given letters from A to F, although several of them have since been resolved into more than one star. Star C was shown to be a binary, but its companion has not been observed. (en)
  • NGC 3603-C (HD 97950C, WR 43c) — спектрально-двойная звезда в центральной части скопления HD 97950 в области звездообразования NGC 3603, расположенной на расстоянии около 25 000 световых лет от Солнца. Первичный компонент принадлежит спектральному классу WN6h и входит в число наиболее массивных и ярких известных звёзд. (ru)
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  • NGC 3603-C (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/NGC3603_core.jpg
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absmag v
  • −7.17 (en)
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  • C is the brightest star to the left of the very close A and B pair at the centre in this HST image of the central region of HD 97950. (en)
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  • WN6h+? (en)
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  • J2000.0 (en)
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