Art

J-GLOBAL ID：202002270124398818   Reference number：20A1045092

Compositions of interstellar molecules at the molecular cloud and galaxy scales

銀河と分子雲スケールで見た星間分子の組成

Author (1)： WATANABE YOSHIMASA (日本大 工)
Material： 低温科学  (Low Temperature Science)
Volume： 78  Page： 211-218  Publication year： Mar. 20, 2020 
JST Material Number： F0327A  ISSN： 1880-7593  Document type： Article
Article type： 原著論文  Country of issue： Japan (JPN)  Language： JAPANESE (JA)

Thesaurus term： *interstellar molecule ,  our galaxy ,  *molecular cloud ,  radiotelescope ,  radio wave observation ,  chemical composition ,  spiral galaxy ,  celestial body
Semi thesaurus term： Galaxy

JST classification (1)： Nebulae  (DB06000W)

Reference (14)：

• Bieging, J. H. et al. (2010), The Arizona Radio Observatory CO Mapping Survey of Galactic Molecular Clouds. I. The W51 Region in CO and ¹³CO J = 2-1 Emission. The Astrophysical Journal Supplement Series, 191, 232-246.
• Harada, N. et al. (2019), Molecular-cloud-scale Chemical Composition. III. Constraints of Average Physical Properties through Chemical Models. The Astrophysical Journal, 871, 238.
• Müller, H. S. P. et al. (2001), The Cologne Database for Molecular Spectroscopy, CDMS. Astronomy and Astrophysics, 370, L49-L52.
• Müller, H. S. P. et al. (2005), The Cologne Database for Molecular Spectroscopy, CDMS: a useful tool for astronomers and spectroscopists. Journal of Molecular Structure, 742, 215-227.
• Nishimura, Y. et al. (2016a), Spectral Line Survey toward Molecular Clouds in the Large Magellanic Cloud. The Astrophysical Journal, 818, 161.

Terms in the title (5)： 銀河 ,  分子雲 ,  スケール ,  星間分子 ,  組成