The Next Generation of High-Mass Stars and Clusters Traced by ATLASGAL - Archive ouverte HAL
Communication Dans Un Congrès Astrophysics and Space Science Proceedings Année : 2014

The Next Generation of High-Mass Stars and Clusters Traced by ATLASGAL

Karl M. Menten
  • Fonction : Auteur
Yanett Contreras
  • Fonction : Auteur
Timea Csengeri
James S. Urquhart
  • Fonction : Auteur
Marion Wienen
  • Fonction : Auteur
Henrik Beuther
Sylvain Bontemps
Leonardo Bronfman
  • Fonction : Auteur
Thomas Henning
Annie Zavagno

Résumé

The Atacama Pathfinder Experiment (APEX) telescope is ideally located to observe the inner part of our Galaxy. With its good sensitivity, the LABOCA bolometer array can map hundreds of square degrees at λ = 870 μ m λ = 870 \upmu m in a reasonable time. ATLASGAL, the APEX Telescope Large Area Survey of the Galaxy, covers 420 deg2 of the inner Galactic plane, with a typical rms noise of 50 mJy/beam. The data reveal thousands of compact sources, as well as giant molecular complexes and large scale filamentary structures. Many follow-up projects are ongoing, and more are planned e.g. with ALMA.
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Dates et versions

hal-00990055 , version 1 (13-05-2014)

Identifiants

Citer

Frédéric Schuller, Karl M. Menten, Friedrich Wyrowski, Yanett Contreras, Timea Csengeri, et al.. The Next Generation of High-Mass Stars and Clusters Traced by ATLASGAL. The Labyrinth of Star Formation, 2012, Greece. pp.421, ⟨10.1007/978-3-319-03041-8_84⟩. ⟨hal-00990055⟩
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