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Daftar bintang paling masif

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Berikut ini adalah daftar bintang paling masif yang pernah ditemukan, dalam satuan Massa Matahari (M).

Ketidakpastian

[sunting | sunting sumber]

Kebanyakan massa yang didaftarkan dibawah masih diperdebatkan, dan, karena masih menjadi subjek penelitian masa kini, masih dalam peninjauan dan sering direvisi massa maupun karakteristiknya yang lain.

  1. ^ Mass is estimated from hydrogen abundance and luminosity, making it very uncertain.
  2. ^ a b c d e f g h i j k l m n o This is a binary system but the secondary is much less massive than the primary.
  3. ^ This unusual measurement was made by assuming the star was ejected from a three-body encounter in NGC 3603. This assumption also means that the current star is the result of a merger between two original close binary components. The mass is consistent with evolutionary mass for a star with the observed parameters.
  4. ^ a b c d e f Mercer 30 is an open cluster in Dragonfish Nebula.
  5. ^ N64 is an emission nebula in Large Magellanic Cloud.
  6. ^ BSDL 1830 is a star cluster in Large Magellanic Cloud.
  7. ^ BSDL 2527 is a star cluster in Large Magellanic Cloud.
  8. ^ BSDL 2505 is a star cluster in Large Magellanic Cloud.
  9. ^ DEM S10 is a H II region in Small Magellanic Cloud.
  10. ^ Bochum 10 is an open cluster in Carina Nebula.
  11. ^ N135 is an emission nebula in Large Magellanic Cloud.
  12. ^ N70 is an emission nebula in Large Magellanic Cloud.
  13. ^ DEM L294 is a H II region in Large Magellanic Cloud.
  14. ^ DEM S80 is a H II region in Small Magellanic Cloud.
  15. ^ a b GKK-A144 is a stellar association in Large Magellanic Cloud.
  16. ^ BSDL 2242 is a star cluster in Large Magellanic Cloud.


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