LEGO - II. A 3 mm molecular line study covering 100 pc of one of the most 
actively star-forming portions within the Milky Way disc

Barnes, A.T.; Kauffmann, J.; Bigiel, F.; Brinkmann, N.; Colombo, D.; Guzmán, A.E.; Kim, W.J.; Szűcs, L.; Wakelam, V.; Aalto, S.; Albertsson, T.; Evans, N.J.; Glover, S.C.O.; Goldsmith, P.F.; Kramer, C.; Menten, K.; Nishimura, Y.; Viti, S.; Watanabe, Y.; Weiss, A.; Wienen, M.; Wiesemeyer, H.; Wyrowski, F.

doi:10.1093/mnras/staa1814

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LEGO - II. A 3 mm molecular line study covering 100 pc of one of the most actively star-forming portions within the Milky Way disc

MPS-Authors

Colombo, D.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Menten, K.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Weiss, A.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Wienen, M.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Wiesemeyer, H.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Wyrowski, F.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Barnes, A., Kauffmann, J., Bigiel, F., Brinkmann, N., Colombo, D., Guzmán, A., et al. (2020). LEGO - II. A 3 mm molecular line study covering 100 pc of one of the most actively star-forming portions within the Milky Way disc. \mnras, 497(2), 1972-2001. doi:10.1093/mnras/staa1814.

Cite as: https://hdl.handle.net/21.11116/0000-0008-43C7-C

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