Data di Pubblicazione:
2016
Abstract:
Context. The HF molecule has been proposed as a sensitive tracer of diffuse interstellar gas, while at higher densities its abundance could be influenced heavily by freeze-out onto dust grains.
Tipologia CRIS:
01.01 Articolo in rivista
Keywords:
ISM: molecules; ISM: clouds; ISM: individual objects: NGC 6334; stars: formation; circumstellar matter; astrochemistry
Elenco autori:
Satta, Mauro
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