A Study of Interstellar Dust Grains based on the Diffuse Galactic Light

基于漫射银河光的星际尘埃颗粒研究

• 批准号: 06640347
• 负责人: ONAKA Takashi
• 金额: $ 1.34万
• 依托单位: The University of Tokyo
• 依托单位国家: 日本
• 项目类别: Grant-in-Aid for General Scientific Research (C)
• 财政年份: 1994
• 资助国家: 日本
• 起止时间: 1994 至 1995
• 项目状态: 已结题
• 来源: https://kaken.nii.ac.jp/en/grant/KAKENHI-PROJECT-06640347/
• 关键词: interstellar material; infrared observation; interstellar grains; polarization; background radiation; space observation

We had a successful mission of the IRTS (InfraRed Telescope in Space), which was launched by the HII-3 rocket on March 18,1995. The IRTS observed about 7 resolution spectra of the diffuse Galactic light by the Mid-InfraRed Spectrometer (MIRS) aboard the IRTS.These provide the mid-IR spectra of the zodiacal light and the diffuse Galactic Light for the first time. We prepared several pieces of software prior to the launch in order to make the observation plan and confirm the flight performance of the MIRS.Based on the post-flight data analysis, we have clearly shown that the mid-infrared diffuse light around the Galactic plane consists of the so-called infrared unidentified bands (UIRs) of the 6.2,7.7,8.6, and 11.3 mm. This suggests the ubiquitous existence of the UIR emitting material in the interstellar space, which is thought to be carbonaceous material and provides key information for the investigation of the interstellar dust grain models. Together with the MIRS data reduction, we have analyzed the COBE data, finding that the mid-IR diffuse emission is proportional to the strength of the interstellar radiation field, which supports the temperature-fluctuating very small dust grain model for this emission. In parallel to this research, we have also shown that the polarization of the thermal emission could provide the information to separate the diffuse emission into several components. In summary, we have clearly established the new observational method for the research of interstellar dust grains by using the diffuse background emission and achieved the primary goal of this project. We are planning to make further analysis of the MIRS data and pursue the investigation of interstellar dust grains.

1995年3月18日，我们成功地完成了由HII-3火箭发射的IRTS（太空中的红色望远镜）的使命。利用IRTS上的中红外光谱仪（MIRS），IRTS观测到了大约7个分辨率的漫射银河光光谱，首次提供了黄道光和漫射银河光的中红外光谱。为了制定观测计划和确认MIRS的飞行性能，我们在发射前准备了几个软件，根据飞行后的数据分析，我们清楚地表明，银河平面周围的中红外漫射光由6.2，7.7，8.6，这表明星际空间中普遍存在UIR发射材料，这被认为是碳质材料，并为星际尘埃颗粒模型的研究提供了关键信息。结合MIRS数据处理，我们分析了COBE数据，发现中红外漫辐射与星际辐射场的强度成正比，这支持了温度波动的极小尘埃颗粒模型。在这项研究的同时，我们还表明，偏振的热发射可以提供的信息，分离成几个组件的漫发射。综上所述，我们明确建立了利用漫射背景辐射研究星际尘埃颗粒的新观测方法，实现了本项目的初步目标。我们正计划对MIRS数据进行进一步分析，并对星际尘埃颗粒进行调查。

项目成果

J.Bock, et al.: ""Performance of a Cooled Baffle System for Space-borne Infrared Telescopes"" Applied Optics. 34. 2268-2277 (1995)

J.Bock 等人：“星载红外望远镜冷却挡板系统的性能”应用光学。

T.Onaka: "Polalrization of Thermal Emission from Aspherical Dust Grains in an Anisotropic Radiation Field" The Astrophysical Journal. 439. L21-L24 (1995)

T.Onaka：“各向异性辐射场中非球面尘埃颗粒热发射的偏振”《天体物理学杂志》。

H.Izumiura,et al.: "SiO Maser Survey of the Galactic Bulge IRAS Sources:II.The4<=b=<5 Strips" The Astrophysical Journal Supplement. 98. 271-204 (1995)

H.Izumiura 等人：“银河系核球 IRAS 来源的 SiO 脉泽勘测：II.The4<=b=<5 条带”天体物理学杂志增刊。

J.J.Bock et al.: "Cooled Baffle System for Space-borne Infrared Telescopes" Applied Optics. (印刷中). (1995)

J.J.Bock 等人：“星载红外望远镜的冷却挡板系统”（正在出版）。

T.Onaka: "Polarization of Thermal Emission from Aspherical Dust Grains in an Anisotropic Radiation Field" The Astrophysical Journal. (印刷中). (1995)

T. Onaka：“各向异性辐射场中非球面尘埃颗粒的热发射的偏振”《天体物理学杂志》（1995 年出版）。