Study on the Activities and Interactions of Galaxies Based on the Observations at the Astronomical Observatories in Chile

基于智利天文台观测的星系活动和相互作用研究

• 批准号: 62043046
• 负责人: NISHIDA Minoru
• 金额: $ 0.7万
• 依托单位: Kyoto University
• 依托单位国家: 日本
• 项目类别: Grant-in-Aid for Overseas Scientific Research
• 财政年份: 1986
• 资助国家: 日本
• 起止时间: 1986 至 1987
• 项目状态: 已结题
• 来源: https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-62043046/
• 关键词: Galaxies; active galactic Nuclei

1. UBVRI Photometry of Merging Galaxies and Optical Identifications of IRAS Objects in the Rho Ophiuchus Molecular Cloud Complex (M. Nishida and T. Ichikawa) From May 29 to 31, 1986, UBVRI photometry of merging galaxies was done by using ASCAP(Automated Single Channel Aperture Photometer) on the 1.0m telescope at CTIO (Cerro Tololo Inter-American Observatory, National Optical Astromy Observatories). From June 2 to 6, 1986, to identify the optical objects with the IRAS point sources in the Rho Ophiuchus molecular cloud complex, observations were done by using the Curtis/Schmidt telescope.2.Deep Survey of Quasars (J. Jugaku) From November 25 to December 6, 1986, deep survey observations to serach quasars were done using IIIaF planes on the Curtis/Schmidt telescope at CTIO. Analysis of the plates is in progress.3.Near Infrared Spectroscopy of Active Galactic Nuclei and Merging Galaxies (M. Nishi- da and Y. Taniguchi) From January 9 to 13, 1987, near infrared spectroscopy of galaxies with active galactic nuclei and starbrust nuclei was done by using IRS (Infrared Spectrometer) on the 1.5m telescope at CTIO. h_2 v+1-0 s(1) 2.12 <mu>m, Brackett <alpha>(4.05 <mu>m) and <delta> (2.17 <mu>m), and (Fe II) 1.644 <mu>m emission lines were measured.4.High-Dispersion Spectroscopy of Active Galactic Nuclei and Quasars (M. Iye) From Junuary 20 to February 1, 1987, the high-dispersion spectroscopy of active galactic nuclei and quasars was done by using Boller and Chivens Spectrograph on the 2.2m telescope at ESO(European Southern Observatory), La Silla. Analysis of the data is in progress.

1. 合并星系UBVRI光度测量和Rho蛇夫座分子云复合体中IRAS天体的光学识别（M. Nishida和T. Ichikawa） 1986年5月29日至31日，在CTIO（托洛洛山）1.0m望远镜上使用ASCAP（自动单通道孔径光度计）对合并星系进行UBVRI光度测量 美洲天文台、国家光学天文台）。 1986年6月2日至6日，为了识别Rho Ophiuchus分子云复合体中的IRAS点源光学物体，使用柯蒂斯/施密特望远镜进行了观测。2.类星体深巡天（J. Jugaku） 1986年11月25日至12月6日，使用柯蒂斯/施密特望远镜上的IIIaF平面对类星体进行了深巡天观测。 首席信息官。板块分析正在进行中。 3.活动星系核和合并星系的近红外光谱（M. Nishida 和 Y. Taniguchi） 1987 年 1 月 9 日至 13 日，利用 CTIO 1.5 m 望远镜上的 IRS（红外光谱仪）对具有活动星系核和星暴核的星系进行了近红外光谱分析。测量了h_2 v+1-0 s(1) 2.12 <mu>m、Brackett <alpha>(4.05 <mu>m)和<delta>(2.17 <mu>m)以及(Fe II) 1.644 <mu>m发射线。 4.活动星系核和类星体(M. Iye)的高色散光谱 1月20日至2月1日， 1987年，利用拉西拉欧洲南方天文台2.2m望远镜上的Boller和Chivens摄谱仪对活动星系核和类星体进行了高色散光谱分析。数据分析正在进行中。