Titlebook: A Few Tens au Scale Physical and Chemical Structures Around Young Low-Mass Protostars; Yoko Oya Book 2022 Springer Nature Singapore Pte Lt

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Roger Gariepy M.D., F.R.C.S. (C)The observational data with Atacama Large Millimeter/submillimeter Array (ALMA) is utilized to study physical and chemical structures of low-mass protostellar sources in the following chapters. This chapter describes the principles of an aperture synthesis with an interferometer and the basic features of ALMA.

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Yoko OyaNominated as an outstanding Ph.D. thesis by the Department of Physics at the University of Tokyo.Presents simplified models which clearly describe well the disk.Shares a unified picture of chemical di

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Femoral Neck and Femoral Shaft Surgery,ss of the Universe, they form rich structures in the Universe from large scales (clusters of galaxies and galaxies) to small scales (stars and planets). Among such hierarchical structure, stars are the most fundamental physical elements in the Universe. They also play important roles in chemical evo

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https://doi.org/10.1007/978-3-642-65563-0tacama Large Millimeter/submillimeter Array. The observed lines are investigated to characterize the geometrical configuration of the outflow/envelope system of this source. The CS emission traces both an envelope component extending along the north-south direction and a faint outflow component with

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https://doi.org/10.1007/978-3-642-65563-0oud with Atacama Large Millimeter/Submillimeter Array. A compact component concentrated in the vicinity of the protostar has been detected as well as a well-collimated outflow cavity extending along the northeast-southwest axis. The inclination angle of the outflow is found to be about . based on th

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https://doi.org/10.1007/978-3-319-65220-7. A clear chemical differentiation is seen; OCS and H.CS show an extended distribution with a slight rotation signature, while CH.OH and HCOOCH. are concentrated near the protostar. The extended component is interpreted by the infalling-rotating envelope model with a nearly face-on configuration. Th

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