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What Is Controlling the Fragmentation in the Infrared Dark Cloud G14.225-0.506?: Different Levels of Fragmentation in Twin Hubs.

MPS-Authors

Busquet,  G.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Estalella,  R.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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

Liu,  H.B.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Zhang,  Q.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Girart,  J.M.
Max Planck Institute for Radio Astronomy, Max Planck Society;

de Gregorio-Monsalvo,  I.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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

Anglada,  G.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Ho,  P.T.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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引用

Busquet, G., Estalella, R., Palau, A., Liu, H., Zhang, Q., Girart, J., de Gregorio-Monsalvo, I., Pillai, T., Anglada, G., & Ho, P. (2016). What Is Controlling the Fragmentation in the Infrared Dark Cloud G14.225-0.506?: Different Levels of Fragmentation in Twin Hubs. Astrophysical Journal, 819:, pp. 139. doi:10.3847/0004-637X/819/2/139.


引用: https://hdl.handle.net/11858/00-001M-0000-002E-1586-1
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