EUV observations show hot prominence spicules generated by turbulence in cool solar filaments that may channel mass into the corona and aid filament evaporation.
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A review summarizing observations of star formation and gas relations from molecular clouds to entire galaxies, with updated rate calculation prescriptions.
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Hot prominence spicules launched from turbulent cool solar prominences
EUV observations show hot prominence spicules generated by turbulence in cool solar filaments that may channel mass into the corona and aid filament evaporation.
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Star Formation in the Milky Way and Nearby Galaxies
A review summarizing observations of star formation and gas relations from molecular clouds to entire galaxies, with updated rate calculation prescriptions.