Feb 13, 2008 · We show that the masses of WNH stars are systematically higher than H-poor WR stars (both WN and WC), with little overlap, while H mass fractions of luminous WNH stars …

Sep 18, 2017 · The luminous blue variable (LBV) phase of evolution, punctuated by eruptive mass loss, is thought to be important in the mass-loss evolution of massive stars [1,2]. However, the …

WNh与LBV之间也不是绝对的，它们甚至能互相转化. R136a1色，你值得拥有（图片为56000K（R136a1表面温度）的物体用肉眼观察的颜色） 很好的资料。 看来大麦哲伦云中的 …

(1) LBVs are presumed to represent a brief transitional phase in the evolution of the most massive stars, between the main-sequence O-type stars and the H-deficient Wolf–Rayet (WR) stars. A …

We propose the new designation ‘‘WNH’’ for luminous Wolf-Rayet (WR) stars of the nitrogen sequence with hydrogen in their spectra. These have been commonly referred to as WNL …

We propose the new designation “WNH” for luminous Wolf-Rayet (WR) stars of the nitrogen sequence with hydrogen in their spectra. These have been commonly referred to as WNL …

We propose the new designation "WNH" for luminous Wolf-Rayet (WR) stars of the nitrogen sequence with hydrogen in their spectra. These have been commonly referred to as WNL …

We propose the new designation "WNH" for luminous Wolf-Rayet (WR) stars of the nitrogen sequence with hydrogen in their spectra. These have been commonly referred to as WNL …

We propose the new designation “WNH” for luminous Wolf-Rayet (WR) stars of the nitrogen sequence with hydrogen in their spectra. These have been commonly referred to as WNL …

Feb 12, 2008 · We show that the masses of WNH stars are systematically higher than H-poor WR stars (both WN and WC), with little overlap, while H mass fractions of luminous WNH stars …