An uncertainty principle for star formation – III. The characteristic emission time-scales of star formation rate tracers

ABSTRACT We recently presented a new statistical method to constrain the physics of star formation and feedback on the cloud scale by reconstructing the underlying evolutionary timeline. However, by itself this new method only recovers the relative durations of different evolutionary phases. To enab...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2020-10, Vol.498 (1), p.235-257
Main Authors: Haydon, Daniel T, Kruijssen, J M Diederik, Chevance, Mélanie, Hygate, Alexander P S, Krumholz, Mark R, Schruba, Andreas, Longmore, Steven N
Format: Article
Language:English
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