천문학회보 (The Bulletin of The Korean Astronomical Society)
- 제42권2호
- /
- Pages.43.3-43.3
- /
- 2017
- /
- 1226-2692(pISSN)
Three-Dimensional Structure of Star-Forming Regions in NGC 6822 Hubble V
- Lee, Hye-In (School of Space Research, Kyung Hee University) ;
- Oh, Heeyoung (Korea Astronomy & Space Science institute) ;
- Le, Huynh Anh N. (Department of Physics and Astronomy, Seoul National University) ;
- Pak, Soojong (School of Space Research, Kyung Hee University) ;
- Lee, Sungho (Korea Astronomy & Space Science institute) ;
- Mace, Gregory (Department of Astronomy, the University of Texas) ;
- Jaffe, Daniel T. (Department of Astronomy, the University of Texas) ;
- Nguyen-Luong, Quang (Korea Astronomy & Space Science institute) ;
- Tatematsu, Ken'ichi (National Astronomical Observatory of Japan)
- 발행 : 2017.10.10
초록
NGC 6822 is a dwarf irregular galaxy in the Local Group and it is located in 500 kpc, further than the Large Magellanic Cloud and the Small Magellanic Cloud. Therefore, we can study star-forming processes by local condition in NGC 6822 instead of tidal force of the Galactic gravitational field. Hubble V is the brightest of several H II complexes in this galaxy. We observed Hubble V by using IGRINS attached on the 2.7 m telescope at the McDonald Observatory in Texas, US in May 2016. We performed a spectral mapping of
키워드