Sub-kpc star-formation law in the local luminous infrared galaxy IC 4687 as seen by ALMA
M. Pereira-Santaella, L. Colina, S. Garc\'ia-Burillo, P. Planesas, A., Usero, A. Alonso-Herrero, S. Arribas, S. Cazzoli, B. Emonts, J. Piqueras, L\'opez, M. Villar-Mart\'in

TL;DR
This study investigates the star-formation law at 250 pc scales in the luminous infrared galaxy IC 4687, revealing rapid star formation efficiency and suggesting a bimodal star-formation law that varies with local conditions.
Contribution
First spatially resolved analysis of the star-formation law at 250 pc scales in a starburst LIRG, combining ALMA, HST, and VLT data to explore star formation efficiency.
Findings
IC 4687 forms stars very efficiently with a depletion time of 160 Myr.
A bimodal star-formation law is suggested, differing from normal spirals.
Star formation efficiency does not depend on local dynamical time at these scales.
Abstract
We analyze the spatially resolved (250 pc scales) and integrated star-formation (SF) law in the local luminous infrared galaxy (LIRG) IC4687. This is one of the first studies of the SF law on a starburst LIRG at these small spatial scales. We combined new interferometric ALMA CO(2-1) data with existing HST/NICMOS Pa narrow-band imaging and VLT/SINFONI near-IR integral field spectroscopy to obtain accurate extinction corrected SF rate (SFR) and cold molecular gas surface densities ( and ). We find that IC4687 forms stars very efficiently with an average depletion time () of 160 Myr for the individual 250 pc regions. This is approximately one order of magnitude shorter than the of local normal spirals and also shorter than that of main-sequence high-z objects, even when we use a Galactic conversion factor. This result…
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