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This is a list of the most massive stars that have been discovered, ... 100,000 spectroscopy: SIMBAD [63] [53] [q] Brey 32 B NGC 1966: 62 165,000 12.32 combined : 43,600
Widely recognised as being among the largest known stars, [19] radius decreased to ~500 R ☉ during the 2020 great dimming event. [71] R Horologii: 635 [56] L/T eff: A red giant star with one of the largest ranges in brightness known of stars in the night sky visible to the unaided eye. Despite its large radius, it is less massive than the Sun.
Its core has undergone a contraction known as "core collapse" and it has a central density cusp with an enormous number of stars surrounding what may be a central black hole. [12] Home to over 100,000 stars, [11] the cluster is notable for containing a large number of variable stars (112) and pulsars (8), including one double neutron star ...
100,000 The proper motion of stars across the celestial sphere, which results from their movement through the Milky Way, renders many of the constellations unrecognizable. [33] 100,000 [note 1] The red hypergiant star VY Canis Majoris will likely have exploded in a supernova. [34] 100,000
This is a list of hottest stars so far discovered (excluding degenerate stars), ... 100,000 34 1,122,000 WN4-s: 21,900 [12] NGC 6822-WR 12: 100,000 36 1,288,000 WN4
The following is a list of particularly notable actual or hypothetical stars that have their own articles in Wikipedia, but are not included in the lists above. BPM 37093 — a diamond star Cygnus X-1 — X-ray source
Star formation is the process by which dense regions within molecular clouds in interstellar space, ... each with more than 100,000 ...
Stars that would be brighter than this shed their outer layers so rapidly that they remain hot supergiants after they leave the main sequence. The majority of red supergiants were 10-15 M ☉ main sequence stars and now have luminosities below 100,000 L ☉, and there are very few bright supergiant (Ia) M class stars. [22]