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4.7. The CO 2–1/1–0 ratio in the disk and center of the Milky Way Galaxy
Published online by Cambridge University Press: 25 May 2016
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We are conducting a survey of the CO J=2-1 line emission in the southern Milky Way (the Tokyo-Onsala-ESO-Calán Galactic CO survey), using the 60-cm radio telescope (VST2) in La Silla, Chile. It is combined with the northern survey made with the identical telescope (VST1) at Nobeyama (e.g., Sakamoto et al. 1995), and is directly comparable with the Columbia survey of the CO J=1-0 emission (e.g., Dame et al. 1987).
- Type
- Part II. Nuclear Interstellar Medium
- Information
- Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 179 - 180
- Copyright
- Copyright © Kluwer 1998
References
Dame, T. M., Ungrechts, H., Cohen, R. S., de Geus, E. J., Grenier, I.A., May, J., Murphy, D. C., Nyman, L. Å., & Thaddeus, P. (1987) A composite CO survey of the entire Milky Way, ApJ, 322, pp. 706–720.CrossRefGoogle Scholar
Oka, T., Hasegawa, T., Hayashi, M., Handa, T., & Sakamoto, S. (1997) CO (J=2-1) line observations of the Galactic center molecular cloud complex. II. Dynamical structure and physical conditions, ApJ
in press.CrossRefGoogle Scholar
Sakamoto, S., Hasegawa, T., Hayashi, M., Handa, T., & Oka, T. (1995) An out-of-plane CO (J=2-1) survey of the Milky Way. I. The data, ApJS, 100, pp. 125–131.CrossRefGoogle Scholar
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