
doi: 10.1086/163112
On a construit un modele pour la region de photodissociation d'Orion. Il permet de rendre compte de l'emission observee dans les raies de structure fine de O I a 63 μm et a 145 μm, de C I a 609 μm et C II a 158 μm et des raies rotationnelles de CO. Il explique egalement l'emission H 2 1-0 S(1) etendue, les raies de recombinaison du carbone et la raie C I 9850 A
| selected citations 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). | 213 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Top 1% | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Top 1% | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Top 10% |
