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ABSTRACT The current generation of (sub)mm-telescopes has allowed molecular line emission to become a major tool for studying the physical, kinematic, and chemical properties of extragalactic systems, yet exploiting these observations requires a detailed understanding of where emission lines originate within the Milky Way. In this paper, we present 60 arcsec (∼3 pc) resolution observations of many 3 mm band molecular lines across a large map of the W49 massive star-forming region (∼100 pc × 100 pc at 11 kpc), which were taken as part of the ‘LEGO’ IRAM-30m large project. We find that the spatial extent or brightness of the molecular line transitions aremore »
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Eden, D J ; Liu, Tie ; Kim, Kee-Tae ; Juvela, M ; Liu, S-Y ; Tatematsu, K ; Francesco, J. Di ; Wang, K ; Wu, Y ; Thompson, M A ; et al ( , Monthly Notices of the Royal Astronomical Society)