Zobrazeno 1 - 2
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pro vyhledávání: '"Shang-ruei Wu"'
Autor:
Shang-ruei Wu, 吳尚叡
102
Carbon dioxide (CO2) is one of the most abundant molecules present in interstellar ice after H2O and CO. In the high mass protostars, CO2 represents an important tracer of the chemical and physical history. Further, the photoprocess of CO2 i
Carbon dioxide (CO2) is one of the most abundant molecules present in interstellar ice after H2O and CO. In the high mass protostars, CO2 represents an important tracer of the chemical and physical history. Further, the photoprocess of CO2 i
Externí odkaz:
http://ndltd.ncl.edu.tw/handle/54089630063516185863
Autor:
T. S. Yih, C. Y. Robert Wu, Wei Jie Hu, Jun Ming Qiu, Hok Sum Fung, Michel Nuevo, C. C. Chu, Wing-Huen Ip, Y.-J. Chen, Shang Ruei Wu
Publikováno v:
Astrobiology. 14:119-131
The detection of nucleobases, the informational subunits of DNA and RNA, in several meteorites suggests that these compounds of biological interest were formed via astrophysical, abiotic processes. This hypothesis is in agreement with recent laborato
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a4c8bb4e8519c1961909f670158a7889
https://doi.org/10.1089/ast.2013.1093
https://doi.org/10.1089/ast.2013.1093
