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- W1651947971 abstract "The nebula, G2.4+1.4, is shown to be a highly reddened, photoionised, mass-loss bubble of very high excitation powered by WR 102, the most extreme oxygen sequence Wolf-Rayet star known. It lies at a distance of 3±1kpc, and is about 11 pc in diameter. The exciting star, contains neither hydrogen nor helium in its atmosphere, is losing mass at a velocity of 5530 km.s -1 , and has the following properties: log ( T ion ) = 5.20±0.05; log ( R/R ⊙ ) = 0.05±0.20; log ( L/L ⊙ ) = 5.85±0.20. We conclude that the star is the ~20M ⊙ core of a supermassive star (M ≤ 60M ⊙ ) seen near the end of its life." @default.
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- W1651947971 date "1991-01-01" @default.
- W1651947971 modified "2023-10-14" @default.
- W1651947971 title "G2.4+1.4: An Extraordinary Mass-Loss Bubble Driven by an Extreme WO Star" @default.
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- W1651947971 doi "https://doi.org/10.1017/s0074180900045460" @default.
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