Mapping the Spiral Structure of the Milky Way Galaxy at 21cm Wavelength Using the SALSA Radio Telescope of Onsala Space Observatory
作者： Tarif Rashid Santo , Syed Ashraf Uddin
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摘要: The spiral arms of M ilky Way can be observed at a rest wavelength 21cm emission that is produced by the hyperfine transition electrons in atomic hydrogen. An observation was carried out from galactic longitude 0° to 225° plane. Using velocity components hydrogen clouds locating different longitudes, as function distance center galaxy, were plotted. whole frequency switching mode using remotely operated SA LSA-Onsala 2.3m Radio Telescope located Onsala Space Observatory, Sweden.
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chalmers.se参考文章(5)
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