LBT spectra of 16 stars
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The diffuse interstellar bands (DIBs) at 9577 and 9632{AA} are attributed to electronic transitions of the C60+ fullerene ion; thus, its column density in molecular clouds may...
弥散星际带（diffuse interstellar bands，DIBs）在9577埃与9632埃（Å）处的谱线，被归因于C₆₀⁺富勒烯阳离子的电子跃迁；因此，其在分子云中的柱密度或可……
