Item

ITEM ACTIONS

This item is discarded!DetailsSummary

Discarded

Journal Article

An uncertainty principle for star formation – II. A new method for characterizing the cloud-scale physics of star formation and feedback across cosmic history

MPS-Authors

/persons/resource/persons49238

Kruijssen, J. M. Diederik
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons145964

Schruba, Andreas
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons135142

Hu, Chia-Yu
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

Kruijssen, J. M. D., Schruba, A., Hygate, A. P. S., Hu, C.-Y., Haydon, D. T., & Longmore, S. N. (2018). An uncertainty principle for star formation – II. A new method for characterizing the cloud-scale physics of star formation and feedback across cosmic history. Monthly Notices of the Royal Astronomical Society, 479(2), 1866-1952. doi:10.1093/mnras/sty1128.

Abstract

There is no abstract available