A far-infrared/submillimeter kilometer-baseline interferometer in space

作者: Martin Harwit , David Leisawitz , Stephen Rinehart

DOI: 10.1016/J.NEWAR.2005.11.030

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摘要: Abstract Through the continuing development of improved detectors and detector arrays, far-infrared/submillimeter astronomical space missions have had enormous successes in recent years. Despite these advances, diffraction-limited angular resolving power has remained virtually constant. The advent telescopes with apertures several meters, will improve situation, but still leave image resolution many orders magnitude poorer than most other spectral ranges. After making scientific case for high spatial imaging this range, use interferometry as immediate way producing results, we review interferometers to provide insight on formation first stars.

参考文章(5)
A. Heger, S. E. Woosley, The Nucleosynthetic Signature of Population III The Astrophysical Journal. ,vol. 567, pp. 532- 543 ,(2002) , 10.1086/338487
Tom Abel, Greg L Bryan, Michael L Norman, The Formation of the First Star in the Universe Science. ,vol. 295, pp. 93- 98 ,(2002) , 10.1126/SCIENCE.1063991
R. Schneider, A. Ferrara, R. Salvaterra, Dust formation in very massive primordial supernovae Monthly Notices of the Royal Astronomical Society. ,vol. 351, pp. 1379- 1386 ,(2004) , 10.1111/J.1365-2966.2004.07876.X
W. H. Baumgartner, M. Loewenstein, D. J. Horner, R. F. Mushotzky, Intermediate-Element Abundances in Galaxy Clusters The Astrophysical Journal. ,vol. 620, pp. 680- 696 ,(2005) , 10.1086/427158
Hiromi Mizusawa, Ryoichi Nishi, Kazuyuki Omukai, H_2 Line Emission Associated with the Formation of the First Stars arXiv: Astrophysics. ,(2004) , 10.1093/PASJ/56.3.487