The Next Generation of High-Mass Stars and Clusters Traced by ATLASGAL
Langue
en
Communication dans un congrès
Ce document a été publié dans
Astrophysics and Space Science Proceedings, 2014ASSP...36..421S - The Labyrinth of Star Formation, held in Greece, june 2012, Astrophysics and Space Science Proceedings, Volume 36. ISBN 978-3-319-03040-1. Springer International Publishing Switzerland, p. 421, 2014, 2014ASSP...36..421S - The Labyrinth of Star Formation, held in Greece, june 2012, Astrophysics and Space Science Proceedings, Volume 36. ISBN 978-3-319-03040-1. Springer International Publishing Switzerland, p. 421, 2014, 2012. 2014, vol. 36, p. 421
Springer
Résumé en anglais
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 = ...Lire la suite >
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.< Réduire
Mots clés en anglais
Physics
Origine
Importé de halUnités de recherche