减至最低
发表于 2025-4-1 02:20:49
Molecular Clouds in Regions of Massive Star Formationar neighborhood (G0≈ 1.6×10. erg s. cm.). Furthermore, massive stars also have supersonic winds with velocities up to several thousand km/s carrying between 0.1 and 1% of the star’s luminosity in form of kinetic energy. At the end of its lifetime an 0 star explodes as a supernova, ejecting 10. erg o
PAEAN
发表于 2025-4-1 10:01:25
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