Abstract
We have made high resolution mapping observations of 12CO ( J=l−0) and 13CO ( J=l−0) from the central few hundred parsecs of the Galaxy using the NRO 45m telescope (HPBW=16″). The high resolution CO maps reveal many molecular arc and/or shell structures which could have resulted from interactions with supernovae. We also found a large (radius ∼ 50 pc) ring structure surrounding the region of diffuse X-ray emission, expanding at V EXP ≃ 200 km s−1. This and other evidence suggest that a galactic superwind following a burst of star formation in the recent past is sweeping up the ambient gas. The Galactic center may have experienced a burst of star formation ∼ 5 × 107 years ago, and it may be in post-starburst phase now.
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Oka, T., Hasegawa, T., Handa, T., Sato, F., Tsuboi, M. (1997). CO Mapping of the Inner Few Hundred Parsecs of the Galaxy. In: Latter, W.B., Radford, S.J.E., Jewell, P.R., Mangum, J.G., Bally, J. (eds) CO: Twenty-Five Years of Millimeter-Wave Spectroscopy. International Astronomical Union / Union Astronomique Internationale, vol 170. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5414-7_13
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DOI: https://doi.org/10.1007/978-94-011-5414-7_13
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