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- W1632508496 abstract "Les flux UV, Hα et HI publies sont utilises pour etudier la formation stellaire au travers du disque de la galaxie M81. Les flux UV et Hα sont corriges de l'extinction par la poussiere en utilisant le contenu en HI et sont compares aux predictions d'un modele afin d'etablir des contraintes sur la fonction de masse initiale et d'estimer les taux de formation stellaire sur plusieurs aires du disque" @default.
- W1632508496 created "2016-06-24" @default.
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- W1632508496 date "1989-08-01" @default.
- W1632508496 modified "2023-09-23" @default.
- W1632508496 title "Large-scale aspects of current star formation in the disk of Messier 81" @default.
- W1632508496 hasPublicationYear "1989" @default.
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