2026-03-08T07:34:22Z https://jaxa.repo.nii.ac.jp/oai

oai:jaxa.repo.nii.ac.jp:00036652 2023-06-20T22:52:06Z 1887:1890 1896:1898:1899:1991

Understanding Star Formation with the NGST Massimo, ROBBERTO Steven, V. W. BECKWITH NGST will be the most sensitive telescope for thermal infrared observations of theheavens when it is launched in mid-2009. Observations in the thermal infrared portion of the spectrum are important for a number of areas in the evolution of young stars: the very early phases of star formation, the dynamic processes related to mass accretion and outflows, the late evolution of protoplanetary disks, the kinematics of deeply embedded clusters and the study ofHII and PDR regions in the Local Group. NGST will make contributions to all of these areas, and for some it is likely to be the most important tool for study in the next 15 years. 資料番号: SA4585099000 宇宙科学研究所 Institute of Space and Astronautical Science 2000-12 eng departmental bulletin paper https://jaxa.repo.nii.ac.jp/records/36652 0288-433X AA10455137 The Institute of Space and Astronautical Science report. S.P. : Mid- and Far-Infrared Astronomy and Future Space Mission 14 11 18 https://jaxa.repo.nii.ac.jp/record/36652/files/SA4585099.pdf application/pdf 424.4 kB 2020-01-24