High-Resolution Spectroscopy of Evolved Stars: from ISO to HII/L2

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概要

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• The observations by the Short-Wavelength Spectrometer onboard the Infrared SpaceObservatory gave great impetus to the studies of AGB stars. The ISO/SWS has provided high quality, intermediate-resolution spectra covering a broad wavelength range of 2.4{45 μm. Thesedata enable us, for the first time, to perform an extensive study of the outer atmosphere and inner circumstellar regions of AGB stars. Exploration of the undeveloped wavelength regions in the mid-to far-infrared has led to an enormous treasure of dust features. In this review, we particularly focus on the results of the ISO/SWS observations of O-rich objects. We then discuss the possible followup in future missions.

• 宇宙航空研究開発機構の論文

著者

• Issei Yamamura

  The Institute Of Space And Astronautical Science(isas)

• Issei Yamamura

  The Institute Of Space And Astronautical Science (isas)

関連論文

• Simulations of Observations with the Far-Infrared Surveyor: Design Overview and Current Status
• A simulation code for the infrared whole sky survey with the Far-Infrared Surveyor(FIS) on board ASTRO-F
• Water Vapor in AGB Stars
• High-Resolution Spectroscopy of Evolved Stars: from ISO to HII/L2

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