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LBV 1806−20 is a candidate luminous blue variable (LBV) and likely binary star located around 28,000 light-years (8,700 pc) from the Sun, towards the center of the Milky Way. It has an estimated mass of around 36 sola...
质量最大，亮度最高的恒星
ABSTRACT We report near-infrared photometry, spectroscopy, and speckle imaging of the hot, luminous star we identify as candidate LBV 1806-20 1 . We also present photometry and spectroscopy of 3 nearby stars, which ar...
LBV 1806-20位于电波星云G10.0-03的核心，据信它是由恒星风提供动力，是疏散星团1806-20星团的成员。这个星团是银河系最大的电离氢区W31的一部分。1806-20星团由一些极不寻常的恒星组成，包括4颗沃夫–瑞叶星、一些OB星、和γ射线反复爆发源SGR 1806-20（磁星）。
Despite much theoretical and observational progress, there is no known firm upper limit to the masses of stars. Our understanding of the interplay between the immense radiation pressure produced by massive stars in fo...
LBV 1806-20 is a candidate luminous blue variable (LBV) and likely binary star located around 28,000 light-years (8,700 pc) from the Sun, towards the center of the Milky Way. It has an estimated mass of around 36 sola...
H-band infrared image of 1806−20 cluster 1806−20 (originally named the SGR 1806−20 cluster) is a heavily obscured star cluster on the far side of the Milky Way, approximately 28,000 light-years distant. [3] Some sourc...
