Physical conditions of molecular gas in the galactic center

Makoto Nagai, Kunihiko Tanaka, Kazuhisa Kamegai, Tomoharu Oka

研究成果: Article査読

29 被引用数 (Scopus)

抄録

We estimated the physical conditions of molecular gas in the central molecular zone (CMZ) of the Galaxy, using our CO J = 3-2 data obtained with the Atacama Submillimeter Telescope Experiment (ASTE) in conjunction with J = 1-012CO and 13CO data previously observed with the Nobeyama Radio Observatory (NRO) 45 m telescope. The large velocity gradient (LVG) approximation was employed. The distributions of gas density, kinetic temperature, and CO column density were derived as functions of the position and the velocity for the entire coverage of the CO J = 3-2 data. We fairly determined the physical conditions for 69% of data points in the CMZ with ≥ 1 σ CO detections. The kinetic temperature was found to be roughly uniform in the CMZ, while the gas density was higher in the 120 pc star-forming ring than in the outer dust lanes. The physical conditions of high J = 3-2/J = 1-0 features are also discussed.

本文言語English
ページ(範囲)25-31
ページ数7
ジャーナルPublications of the Astronomical Society of Japan
59
1
DOI
出版ステータスPublished - 2007
外部発表はい

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学

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