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ATLASGAL, the APEX Telescope Large Area Survey of the Galaxy

Published online by Cambridge University Press:  21 October 2010

F. Schuller
Affiliation:
MPIfR, Bonn, Germany; email: schuller@mpifr-bonn.mpg.de
K. M. Menten
Affiliation:
MPIfR, Bonn, Germany; email: schuller@mpifr-bonn.mpg.de
F. Wyrowski
Affiliation:
MPIfR, Bonn, Germany; email: schuller@mpifr-bonn.mpg.de
H. Beuther
Affiliation:
MPIA, Heidelberg, Germany
S. Bontemps
Affiliation:
LAB, Bordeaux, France
L. Bronfman
Affiliation:
Univ. de Chile, Santiago, Chile
Y. Contreras
Affiliation:
Univ. de Chile, Santiago, Chile
T. Henning
Affiliation:
MPIA, Heidelberg, Germany
F. Motte
Affiliation:
CEA/DSM/IRFU/SAp, Saclay, France
P. Schilke
Affiliation:
Universität zu Köln, Germany
M. Walmsley
Affiliation:
Osservatorio Astrofisico di Arcetri, Italy
A. Zavagno
Affiliation:
LAM, Marseille, France
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Abstract

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Submillimeter continuum emission traces high molecular column densities and, thus, dense cloud regions in which new stars are forming. Surveys of the Galactic plane in such emission have the potential of delivering an unbiased view of high-mass star formation throughout the Milky Way. Here we present the scope, current status and first results of ATLASGAL, an ongoing survey of the Galactic plane using the Large APEX Bolometer Camera (LABOCA) on the Atacama Pathfinder Experiment (APEX) telescope at the Chajnantor plateau in Chile. Aimed at mapping 360 square degrees at 870 μm, with a uniform sensitivity of 50 mJy/beam, this survey will provide the first unbiased sample of cold dusty clumps in the Galaxy at submillimeter wavelengths. These will be targets for molecular line follow-up observations and high resolution studies with ALMA and the EVLA.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

References

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