Living on the edge of the Milky Way's central molecular zone. G1.3 is the more 
likely candidate for gas accretion into the CMZ

Busch, Laura A.; Riquelme, Denise; Güsten, Rolf; Menten, Karl M.; Pillai, Thushara G.S.; Kauffmann, Jens

doi:10.1051/0004-6361/202244870

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Living on the edge of the Milky Way's central molecular zone. G1.3 is the more likely candidate for gas accretion into the CMZ

MPS-Authors

Busch, Laura A.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Riquelme, Denise
Max Planck Institute for Radio Astronomy, Max Planck Society;

Güsten, Rolf
Max Planck Institute for Radio Astronomy, Max Planck Society;

Menten, Karl M.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Pillai, Thushara G.S.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Kauffmann, Jens
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Citation

Busch, L. A., Riquelme, D., Güsten, R., Menten, K. M., Pillai, T. G., & Kauffmann, J. (2022). Living on the edge of the Milky Way's central molecular zone. G1.3 is the more likely candidate for gas accretion into the CMZ. åp, 668: A183, pp. A183. doi:10.1051/0004-6361/202244870.

Cite as: https://hdl.handle.net/21.11116/0000-000C-C94B-E

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