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1 Introduction
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2 Overview of the region
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3 Observations
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4 Results: 13CO 2 1 and 12CO and 13CO 3 2
mapping
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5 Mid-infrared emission from MSX: probing the association
of molecular clouds with young OB stars and embedded IR sources
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6 Discussion
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7 Summary
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References
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Online Material
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Appendix A: Line integrated maps of 13CO and 12CO 3 2
emission
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Appendix B: Line integrated maps of 13CO 2 1 emission in individual regions
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Appendix C: Clump properties
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