EMISSION LINE VELOCITY FIELD OF THE MAGELLANIC IRREGULAR GALAXY NGC 4449

HIROSHI OHTANI; MAMORU SAITO; KOUJI OHTA; MICHITOSHI YOSHIDA; TASUHlRO SHIMIZU; HISASHI KOYANO; GEORGE KOSUGI; KENTARO AOKI; TOSHIYUKI SASAKI; MINORU SASAKI

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EMISSION LINE VELOCITY FIELD OF THE MAGELLANIC IRREGULAR GALAXY NGC 4449 KCI 등재 SCOPUS

MINORU SASAKI, HIROSHI OHTANI, MAMORU SAITO, KOUJI OHTA, MICHITOSHI YOSHIDA, TASUHlRO SHIMIZU, HISASHI KOYANO, GEORGE KOSUGI, KENTARO AOKI, TOSHIYUKI SASAKI

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URLhttps://db.koreascholar.com/Article/Detail/387812

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천문학회지 (Journal of The Korean Astronomical Society)

제29권 제S호 (1996.12)
pp.85-86

한국천문학회 (Korean Astronomical Society)

초록

The imaging spectroscopic observations of the Magellanic irregular galaxy NGC 4449 were made to show the detailed kinematic structure of the galaxy. Many filamentary structures and Several bubble-like structures are recognized in a 3D data cube of H$\alpha$ 수식 이미지 emission line. Velocity field shows the kpc-scale mosaic structure and counter- rotation of ionized gas.

키워드

irregular galaxies internal motion

저자

HIROSHI OHTANI(Department of Astronomy, Kyoto University)
MAMORU SAITO(Department of Astronomy, Kyoto University)
KOUJI OHTA(Department of Astronomy, Kyoto University)
MICHITOSHI YOSHIDA(Okayama Astrophysical Observatory)
TASUHlRO SHIMIZU(Okayama Astrophysical Observatory)
HISASHI KOYANO(Okayama Astrophysical Observatory)
GEORGE KOSUGI(National Astronomical Observatory)
KENTARO AOKI(National Astronomical Observatory)
TOSHIYUKI SASAKI(National Astronomical Observatory)
MINORU SASAKI(Shimonoseki City University)

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