東京大学・天文学教育研究センターでは2003年4月から談話会を開いています。
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ML: semiadm _at_ ioa.s.u-tokyo.ac.jp
please replace _at_ with @
Language: English
Abstract: This talk will present first results of the MIRI-MRS spectra of a number of protostars, T Tauri and brown dwarf disks resulting from the JOYS and MINDS GTO programs as well as a number of open time programs. Rich ice spectra are seen in dark clouds and the cold outer envelopes of protostars hinting at the presence of complex molecules in ices formed very early in the evolution. In young and mature disks, many lines from gaseous CO, H2O, CO2, C2H2 and HCN are found, but also surprising new molecules are detected. Together they point to a rich chemistry that is linked to the physical structure of the inner regions of these disks and thereby provides a unique diagnostic of it. Background information: the 55 hr JWST Observations of Young protoStars (JOYS) GTO program (PI: van Dishoeck) uses MIRI to investigate the physical and chemical properties of two dozen protostars and their immediate environment. JOYS studies the physical characteristics of embedded disks, accretion signatures onto the protostars, feedback from the young protostars on their environment through primordial jets and outflows, as well as the chemical gas and ice constituents of the protostellar envelopes to feed the disks. The goal of the 120 hr MIRI Mid INfrared Disk Survey (MINDS) GTO program (Th. Henning, I. Kamp co-PIs) is to use JWST to (1) investigate the chemical inventory of the terrestrial planet forming zone, (2) to follow the gas evolution into the disk dispersal stage, and to (3) study the structure of protoplanetary and debris disks in the thermal mid-IR. The program builds a bridge between the chemical inventory of planet-forming disks and the properties of exoplanets. In total, about 50 targets (Herbig Ae stars, T Tauri stars, brown dwarfs and young debris disks) are being observed.
# | Date | Speaker | Title | Chair |
405 | 2023年10月3日(火) 天文学教室との合同談話会 | Ewine van Dishoeck (Leiden Observatory) | Protostars and protoplanetary disks with JWST: first results from the JOYS and MINDS programs | N. Matsunaga |
406 | 2023年10月26日(木) | 平尾優樹 (天文学教育研究センター) | TBA | TBA |
407 | 2023年11月16日(木) | 日下部晴香 (国立天文台・科学研究部) | TBA | TBA |
詳細はこちら: 令和5(2023)年度談話会
# | Date | Speaker | Title | Chair |
403 | 2023年6月8日(木) | 今井正尭 (天文学教育研究センター) | Observations of planetary-scale waves on Venus atmosphere | S. Koyama |
404 | 2023年6月29日(木) | 谷口琴美 (国立天文台・科学研究部) | Chemical complexity around massive young stellar objects revealed by ALMA | K. Kohno |
402 | 2023年5月25日(木) | 藤田真司 Shinji Fujita (Institute of Astronomy, the University of Tokyo) | Distance determination of molecular clouds in the Galaxy using deep learning | M. Imai |
401 | 2023年4月20日(木) | Yao-Lun Yang (Research Scientist, RIKEN) | Complex chemistry in the era of JWST and ALMA | K. Kohno |
400 | 2023年4月6日(木) | Doug Johnstone (National Research Council Canada) | What the Variability of Embedded Protostars Tells Us about Accretion: Past, Present, and Future | K. Kohno |