Spectroscopic Observations of the Star Formation Regions in Nearby Galaxies |
| |
| Authors: | KONG Xu LIN Lin LI Jin-rong ZHOU Xu ZOU Hu LI Hong-yu CHEN Fu-zhen DU Wei FAN Zhou MAO Ye-wei WANG Jing ZHU Yi-nan ZHOU Zhi-min |
| |
| Affiliation: | 1. Center for Astrophysics, University of Science and Technology of China, Hefei 230026;2. Key Laboratory for Research in Galaxies and Cosmology, Chinese Academy of Sciences, Hefei 230026;3. National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012;4. Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008;5. Max Planck Institute for Astrophysics, Garching by Munich D-85741 |
| |
| Abstract: | In recent years the number of worldwide 8∼10 m-class ground-based telescopes is continually increased, the 4 m-diameter or smaller telescopes have become the small and medium-sized telescopes. In order to obtain some noticeable scientific results by using these existing small and medium-sized telescopes, we have to consider very carefully what we can do, and what we can not. For this reason, the Time Allocation Committee of the 2.16 m telescope of the National Astronomical observatories of China (NAOC) has decided to support some key projects since 2013. The long-term project “Spectroscopic Observations of the Star Formation Regions in Nearby Galaxies” proposed by us is one of three key projects, it is supported by the committee with 30 dark/grey nights in each of three years. |
| |
| Keywords: | ISM: dust extinction&mdash galaxies: emission lines&mdash galaxies: kinematics and dynamics&mdash galaxies: star formation |
| 本文献已被 ScienceDirect 等数据库收录！ |
|
