A law for star formation in galaxies
arXiv:1104.3596 · doi:10.1088/0004-637X/735/1/56
Abstract
We study the galactic-scale triggering of star formation. We find that the largest mass-scale not stabilized by rotation, a well defined quantity in a rotating system and with clear dynamical meaning, strongly correlates with the star formation rate in a wide range of galaxies. We find that this relation can be understood in terms of self-regulation towards marginal Toomre stability and the amount of turbulence allowed to sustain the system in this self-regulated quasi-stationary state. We test such an interpretation by computing the predicted star formation rates for a galactic interstellar medium characterized by lognormal probability distribution function and find good agreement with the observed relation.
13 pages, 2 figures, Accepted in ApJ
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- Near-infrared adaptive optics imaging of infrared luminous galaxies: the brightest cluster magnitude - star formation rate relation
- The K-band luminosity functions of super star clusters in luminous infrared galaxies, their slopes, and the effects of blending
- Observational Support for Massive Black Hole Formation Driven by Runaway Stellar Collisions in Galactic Nuclei
- The extended law of star formation: the combined role of gas and stars
- The Interstellar Medium and Star Formation in Local Galaxies: Variations of the Star Formation Law in Simulations
- Gravitational Fragmentation in Galaxy Mergers: A Stability Criteria
- On the Functional Form of the Universal Star Formation Law