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


Ontology type: schema:Chapter     


Chapter Info

DATE

2014-01-28

AUTHORS

Frédéric Schuller , Karl M. Menten , Friedrich Wyrowski , Yanett Contreras , Timea Csengeri , James S. Urquhart , Marion Wienen , Henrik Beuther , Sylvain Bontemps , Leonardo Bronfman , Lise Deharveng , Thomas Henning , Malcolm Walmsley , Annie Zavagno

ABSTRACT

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=870μm\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\lambda = 870\,\upmu \mathrm{m}$$\end{document} 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. More... »

PAGES

421-423

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-3-319-03041-8_84

DOI

http://dx.doi.org/10.1007/978-3-319-03041-8_84

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1031239901


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