High-mass Star Formation through Filamentary Collapse and Clump-fed Accretion 
in G22

Yuan, J.; Li, J.-Z.; Wu, Y.; Ellingsen, S.P.; Henkel, C.; Wang, K.; Liu, T.; Liu, H.-L.; Zavagno, A.; Ren, Z.; Huang, Y.

doi:10.3847/1538-4357/aa9d40

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High-mass Star Formation through Filamentary Collapse and Clump-fed Accretion in G22

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Henkel, C.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Yuan, J., Li, J.-Z., Wu, Y., Ellingsen, S., Henkel, C., Wang, K., et al. (2018). High-mass Star Formation through Filamentary Collapse and Clump-fed Accretion in G22. Astrophysical Journal, 852: 12, pp. 12. doi:10.3847/1538-4357/aa9d40.

Cite as: https://hdl.handle.net/21.11116/0000-0004-3C76-5

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