@inproceedings{oai:jaxa.repo.nii.ac.jp:00003014,
 author = {Tielens, A. G. G. M.},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe},
 month = {Mar},
 note = {SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan, The evolution of the interstellar medium is driven by a number of complex processes which are deeply interwoven, including mass accretion from nearby (dwarf) systems and the intergalactic medium, mass ejection into the halo and interglactic medium, stellar mass injection into the interstellar medium, star formation, mechanical energy input by stellar winds & supernova explosions, and radiative energy input. These processes are mediated by dust and molecules in an only partially understood way. This complex feedback between stars and the medium they are formed in drives the evolution of galaxies and their observational characteristics. SPICA is set to expand studies of the origin and evolution of the interstellar medium and its role in the evolution of galaxies to the era of vigorous star formation in the Universe at redshifts between 1 and 3. Yet, our understanding of what these observations tell us about what really happens at those epochs will depend very much on our understanding of the microscopic physical and chemical processes and their dependence on the local conditions. These are best studied in the local universe. In order to reap the full benefits of SPICA, a concerted program of key observations is required that study the physics and chemistry of the ISM locally and leverage this to probe the far Universe., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027037, レポート番号: JAXA-SP-17-010E},
 pages = {163--171},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {The Cycling of Matter between Stars, the Interstellar Medium, and the Intergalactic Medium},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}