Abstract
La detection de raies de recombinaison du carbone en absorption en direction du Centre Galactique a 75 MHz et en direction de M16 a 68 MHz et 80 MHz est rapportee. En direction de M16, la raie a egalement ete detectee en emission a 325 MHz. Les largeurs des raies impliquent des densites d'electrons inferieures a 0.8 cm −3 dans les nuages absorbants
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