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- W1486822609 abstract "Presentation de nouvelles observations CCD polarimetriques de la region du Serpent et des observations photometriques IR de quelques sources ainsi que des cartes 2,2 μm des champs entourant la nebuleuse reflechissante du Serpent et la source IR SVS4. Une analyse de l'extinction au moyen de la relation de Hubble suggere la presence d'un disque ou d'un tore de poussiere entourant les etoiles excitatrices. L'axe de symetrie principal des nebulosites est correle avec la composante helicoidale du champ magnetique interstellaire; ce resultat est interprete en termes de processus de formation stellaire dans le nuage du Serpent. L'efficacite de la formation stellaire et la densite de masse suggerent la formation d'un amas stellaire" @default.
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- W1486822609 date "1988-08-01" @default.
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- W1486822609 title "Observational evidence for the influence of the magnetic-field on star formation in the serpens molecular cloud" @default.
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