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Characterising the high-mass star forming filament G351.776-0.527 with Herschel and APEX dust continuum and gas observations

MPS-Authors

Pillai,  T.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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

Urquhart,  J.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Csengeri,  T.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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

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

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

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Citation

Leurini, S., Schisano, E., Pillai, T., Giannetti, A., Urquhart, J., Csengeri, T., et al. (2019). Characterising the high-mass star forming filament G351.776-0.527 with Herschel and APEX dust continuum and gas observations. aap, 621: A130, pp. A130. doi:10.1051/0004-6361/201833612.


Cite as: https://hdl.handle.net/21.11116/0000-0006-79FC-7
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