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2007 IPY SYMPOSIUM

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Abstract

TERAHERTZ ASTRONOMY FROM THE COLDEST PLACE ON EARTH

Christopher K. Walker
University of Arizona
Bio

Many atoms and molecules have emission lines that occur at THz frequencies. These emission lines can be used to probe the conditions in Giant Molecular Clouds (GMCs) throughout our galaxy. From studying the star formation process in GMCs we will gain a better under-standing of the origin of planetary systems like our own. The high Antarctic plateau offers unique opportunities for observatories optimized for this important wavelength regime. A new 0.5-meter observatory, the High Elevation Antarctic Terahertz Telescope (HEAT), is being proposed for Dome A in Antarctica. Dome A is the highest (4.1 km), driest, coldest site on the ice plateau. From its summit, observations of the astrophysically important 1.46 and 1.9 THz lines from N+ and C+ should be routinely possible. From remote sites such as Dome A, the next generation of THz instrumentation can be field tested, providing an invaluable dress rehearsal for future space missions.

 

 

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