Icy Origins of Organic Molecules Unveiled by JWST

JWST 揭示了有机分子的冰冷起源

• 批准号: 22K20389
• 负责人: 楊 燿綸
• 金额: $ 1.83万
• 依托单位: Institute of Physical and Chemical Research
• 依托单位国家: 日本
• 项目类别: Grant-in-Aid for Research Activity Start-up
• 财政年份: 2022
• 资助国家: 日本
• 起止时间: 2022-08-31 至 2024-03-31
• 项目状态: 已结题
• 来源: https://kaken.nii.ac.jp/en/grant/KAKENHI-PROJECT-22K20389/
• 关键词: interstellar ice; astrochemistry; low-mass protostars; infrared spectrscopy; Astrochemistry; Ice; Infrared Astronomy

The primary goals of this research program is to measure the ice abundance in four young protostars and test chemical models with radiative transfer calculations, using JWST data. I have been leading the collaboration to develop the method of data reduction and measuring ice column density from its absorption feature. We published the first identification of ice features as well as jet and outflow characterization on the Astrophysical Journal Letter (Yang et al. 2022b). In this article, we presented the first JWST spectrum of a young protostar, identifying both commonly known ice feature as well as the features that could be due to organic molecules, such as ethanol and acetaldehyde. We also demonstrate the unique capability of JWST spectroscopic data on not only ice measurements but also characterizing outflows and jets in young protostars, where such observations were challenging to perform due to high extinction. Moreover, there are a number of projects underway in this project. The detailed ice analysis is led by Dr. J. Kim (KASI) and Mr. C.-H. Kim (SNU) with myself as the main mentor. I also started collaborations with Dr. Salyk (Vasser) and Dr. Okoda (RIKEN) to expand the breath of this research program.

该研究计划的主要目标是使用 JWST 数据测量四颗年轻原恒星的冰丰度，并通过辐射传输计算测试化学模型。我一直在领导合作开发数据简化方法并根据冰柱的吸收特征测量冰柱密度。我们在《天体物理学杂志快报》上发表了对冰特征以及射流和流出特征的首次识别（Yang 等人，2022b）。 在本文中，我们展示了一颗年轻原恒星的第一个 JWST 光谱，识别了众所周知的冰特征以及可能由有机分子（例如乙醇和乙醛）引起的特征。 我们还展示了 JWST 光谱数据的独特功能，不仅可以测量冰，还可以表征年轻原恒星的流出和喷流，而由于高消光，此类观测很难进行。 此外，该项目还有多个项目正在进行中。 详细的冰分析由 J. Kim 博士 (KASI) 和 C.-H 先生领导。 Kim（首尔国立大学），我是主要导师。我还开始与 Salyk 博士（Vasser）和 Okoda 博士（RIKEN）合作，以扩展该研究项目的气息。

项目成果

KASI/Seoul National University(韓国)

KASI/首尔国立大学（韩国）

The JWST View of Ice and Fire in a Class 0 Protostar: The tale of IRAS 15398-3359

JWST 对 0 级原恒星冰与火的看法：IRAS 15398-3359 的故事

• 发表时间: 2022
• 作者: Yao-Lun Yang;鈴木龍汰，瀬谷昇治，長津雄一郎，伴貴彦，Manoranjan Mishra;Yao-Lun Yang;Hiroaki KUSUNO;岩﨑かおり，鈴木龍汰，長津雄一郎，伴貴彦，ミシュラマノランジャン，長津雄一郎;Yao-Lun Yang;楠野宏明;Yao-Lun Yang
• 通讯作者: Yao-Lun Yang

Models of Rotating Infall for the B335 Protostar

B335 Protostar 的旋转瀑布模型

• DOI: 10.3847/1538-4357/acaa38
• 发表时间: 2023
• 期刊: The Astrophysical Journal
• 作者: Evans II Neal J.;Yang Yao-Lun;Green Joel D.;Zhao Bo;Di Francesco James;Lee Jeong-Eun;Jorgensen Jes K.;Choi Minho;Myers Philip C.;Mardones Diego
• 通讯作者: Mardones Diego

Evolution of Organic Chemistry from Ice to Gas: The Synergy between ALMA and JWST

有机化学从冰到气体的演变：ALMA 和 JWST 之间的协同作用

• 发表时间: 2023
• 作者: Yao-Lun Yang

Complex Chemistry in a Class 0 Protostars IRAS 15398-3359

0 级原恒星中的复杂化学 IRAS 15398-3359

• 发表时间: 2022
• 作者: Yao-Lun Yang;鈴木龍汰，瀬谷昇治，長津雄一郎，伴貴彦，Manoranjan Mishra;Yao-Lun Yang;Hiroaki KUSUNO;岩﨑かおり，鈴木龍汰，長津雄一郎，伴貴彦，ミシュラマノランジャン，長津雄一郎;Yao-Lun Yang
• 通讯作者: Yao-Lun Yang