
On a determine les abondances de l'oxygene dans les regions HII de 12 galaxies de faible brillance de surface. On trouve que la plupart ressemblent aux galaxies spirales et irregulieres deja etudiees. La seule exception est la tres grande galaxie barree faible UKS 1348-355 dans laquelle les etoiles ne se sont formees que tres lentement sur une grande region
| 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). | 12 | |
| 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. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
