On the CH(+) ion in diffuse interstellar clouds
Copyright policy ) D. L. Lambert; A. C. Danks;
On the CH(+) ion in diffuse interstellar clouds
Un balayage de 65 lignes de visee dans la Voie Lactee Sud dans la raie interstellaire de CH + a 4232 A a permis 30 detections. La densite de colonne de CH + N(CH + ) est bien correlee avec H 2 excite par rotation detecte par des balayages effectues avec Copernicus. Cette correlation pourrait indiquer que CH + se forme dans du gaz chaud ou la reaction C + +H 2 →CH + +H est effective. Des chocs apportent probablement le chauffage necessaire
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These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
Citations provided by BIP!popularityPopularity provided by BIP!
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
Popularity provided by BIP! 53
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