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Intensity Mapping of the [CII] Fine Structure Line during the Epoch of Reionization
Intensity Mapping Fine Structure Line during Epoch Reionization
2011/10/11
The atomic CII fine-structure line is one of the brightest lines in a typical star-forming galaxy spectrum with a luminosity ~ 0.1% to 1% of the bolometric luminosity. It is potentially a reliable tra...
Radio Continuum and H92 Recombination Line Observations of G34.26+0.15 and G5.89-0.39
G34.26+0.15 G5.89-0.39 H92 Recombination Line
2009/6/11
Radio Continuum and H92 Recombination Line Observations of G34.26+0.15 and G5.89-0.39。
DOUBLY-EXCITED ATOMS AND THE LINE BROADENING。