Daftar bintang paling masif

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

Ketidakpastian

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.

Daftar

Catatan

  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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