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MALT90: tracing the chemistry and kinematics of molecular clumps within the central molecular zone
Published online by Cambridge University Press: 22 May 2014
Abstract
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The MALT90 survey targets more than 2000 high-mass star-forming clumps in the Galactic plane obtaining small maps around each of them, in 16 molecular lines at 90 GHz. By observing several thousand high-mass star forming clumps MALT90 aims to characterize their global chemical and physical evolution. Here we summarize the survey parameters and show examples of the MALT90 data toward three clumps in the central molecular zone.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 9 , Symposium S303: The Galactic Center: Feeding and Feedback in a Normal Galactic Nucleus , October 2013 , pp. 182 - 184
- Copyright
- Copyright © International Astronomical Union 2014
References
Jackson, J. M., Rathborne, J. M., Foster, J. B.et al. 2013, arXiv: 1310.1131, accepted to PASAGoogle Scholar