Documentation scienceplus.abes.fr version Bêta

À propos de : Young stars in the periphery of NGC 6822        

AttributsValeurs
type
Is Part Of
Subject
Title
  • Young stars in the periphery of NGC 6822
Date
has manifestation of work
related by
Author
Abstract
  • Taking advantage of the wide ( $42'\times 28'$) field of the CFH12K camera, we survey the young star population of NGC 6822 to unprecedented radial distances. We determine the age of the young stars by employing Gallart's et al. ([CITE]) method based on the presence of stars in different boxes in the CMD. We find that star formation took place up to ~200 Myr ago in a wide area not always matching the current HI cloud. A ~50 Myr old association is identified, next to the HI void where no young stars are seen.
article type
publisher identifier
  • aa3563
Date Copyrighted
Rights
  • © ESO, 2003
Rights Holder
  • ESO
is part of this journal
is primary topic of



Alternative Linked Data Documents: ODE     Content Formats:       RDF       ODATA       Microdata