THE MILLIMETER ASTRONOMY LEGACY TEAM 90 GHz (MALT90) PILOT SURVEY

被引:112
作者
Foster, Jonathan B. [1 ]
Jackson, James M. [1 ]
Barnes, Peter J. [2 ]
Barris, Elizabeth [1 ]
Brooks, Kate [3 ]
Cunningham, Maria [4 ]
Finn, Susanna C. [1 ]
Fuller, Gary A. [5 ]
Longmore, Steve N. [6 ,7 ]
Mascoop, Joshua L. [1 ]
Peretto, Nicolas [8 ]
Rathborne, Jill [3 ,9 ]
Sanhueza, Patricio [1 ]
Schuller, Frederic [10 ]
Wyrowski, Friedrich [10 ]
机构
[1] Boston Univ, Inst Astrophys Res, Boston, MA 02215 USA
[2] Univ Florida, Dept Astron, Gainesville, FL 32611 USA
[3] CSIRO Astron & Space Sci, Epping, NSW 1710, Australia
[4] Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia
[5] Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Manchester M13 9PL, Lancs, England
[6] ESO Headquarters, D-85748 Garching, Germany
[7] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[8] Univ Paris Diderot, CEA, CNRS, Lab AIM,DSM,IRFU,Serv Astrophys,CE Saclay, F-91191 Gif Sur Yvette, France
[9] Univ Chile, Dept Astron, Santiago, Chile
[10] Max Planck Inst Radioastron, D-53121 Bonn, Germany
基金
澳大利亚研究理事会; 美国国家航空航天局;
关键词
ISM: molecules; stars: formation; stars: massive; surveys; INFRARED DARK CLOUDS; STAR-FORMATION; GALACTIC PLANE; CO SURVEY; CORES; CANDIDATES; TELESCOPE; EMISSION; OUTFLOWS; REGIONS;
D O I
10.1088/0067-0049/197/2/25
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We describe a pilot survey conducted with the Mopra 22 m radio telescope in preparation for the Millimeter Astronomy Legacy Team Survey at 90 GHz (MALT90). We identified 182 candidate dense molecular clumps using six different selection criteria and mapped each source simultaneously in 16 different lines near 90 GHz. We present a summary of the data and describe how the results of the pilot survey shaped the design of the larger MALT90 survey. We motivate our selection of target sources for the main survey based on the pilot detection rates and demonstrate the value of mapping in multiple lines simultaneously at high spectral resolution.
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页数:15
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