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A Portrait of Cold Gas in Galaxies at 60 pc Resolution and a Simple Method to Test Hypotheses That Link Small-scale ISM Structure to Galaxy-scale Processes

MPS-Authors

Leroy,  A.K.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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

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

Rosolowsky,  E.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Blanc,  G.A.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Bolatto,  A.D.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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

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

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

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

Meidt,  S.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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

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

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

Schinnerer,  E.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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

Usero, 
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Citation

Leroy, A., Hughes, A., Schruba, A., Rosolowsky, E., Blanc, G., Bolatto, A., et al. (2016). A Portrait of Cold Gas in Galaxies at 60 pc Resolution and a Simple Method to Test Hypotheses That Link Small-scale ISM Structure to Galaxy-scale Processes. Astrophysical Journal, 831: 16, pp. 16. doi:10.3847/0004-637X/831/1/16.


Cite as: https://hdl.handle.net/11858/00-001M-0000-002E-152C-F
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