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A few tens au scale physical and che...

Oya, Yoko.

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A few tens au scale physical and chemical structures around young low-mass protostars

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	A few tens au scale physical and chemical structures around young low-mass protostars/ by Yoko Oya.
作者:	Oya, Yoko.
出版者:	Singapore :Springer Nature Singapore : : 2022.,
面頁冊數:	xvi, 212 p. :ill. (chiefly color), digital ;24 cm.
附註:	"Doctoral thesis accepted by The University of Tokyo, Tokyo, Japan."
內容註:	Introduction -- ALMA Observation -- Model Calculation -- L1527 -- IRAS 15398-3359 -- IRAS 16293-2422 Source A -- IRAS 16293-2422 Source B -- L483 -- Chemical Differentiation -- Physical Diversity -- Conclusion.
Contained By:	Springer Nature eBook
標題:	Stars - Formation. -
電子資源:	https://doi.org/10.1007/978-981-19-1708-0
ISBN:	9789811917080

A few tens au scale physical and chemical structures around young low-mass protostars
Oya, Yoko.

A few tens au scale physical and chemical structures around young low-mass protostars[electronic resource] /by Yoko Oya. - Singapore :Springer Nature Singapore :2022. - xvi, 212 p. :ill. (chiefly color), digital ;24 cm. - Springer theses,2190-5061. - Springer theses..

"Doctoral thesis accepted by The University of Tokyo, Tokyo, Japan."

Introduction -- ALMA Observation -- Model Calculation -- L1527 -- IRAS 15398-3359 -- IRAS 16293-2422 Source A -- IRAS 16293-2422 Source B -- L483 -- Chemical Differentiation -- Physical Diversity -- Conclusion.

This book characterizes the kinematic and chemical structures of disk-forming regions around low-mass protostellar sources and their interplay based on Atacama Large Millimeter/submillimeter Array (ALMA) observations. It describes the chemical evolution of molecules formed in an interstellar gas using the ALMA observations of 5 Sun-like protostars at a spatial resolution of a few tens au scale, which unveils the physical mechanism of star and planetary formation. The book reviews the author's successful works, focusing on two key findings: (i) A drastic change in the chemical composition of the gas around the centrifugal barrier of the infalling-rotating envelopes, and (ii) the chemical composition in the disk-forming regions, which varies from source to source depending on the chemical characteristics of the parent molecular cloud. These findings are based on the fine characterization of physical structures based on careful kinematic analyses. An additional attraction is the inclusion of the skillful reviews of ALMA observatory and its observation and physical models to describe the observed gas structure.

ISBN: 9789811917080

Standard No.: 10.1007/978-981-19-1708-0doiSubjects--Topical Terms:

777194
Stars
--Formation.

LC Class. No.: QB806

Dewey Class. No.: 523.8

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