papers

Publications (5)

astro-ph.GA2017

CO/CO Gradients Across the Disks of Nearby Spiral Galaxies

M. J. Jimenez-Donaire, D. Cormier, F. Bigiel +14

We use the IRAM Large Program EMPIRE and new high-resolution ALMA data to measure 13CO(1-0)/C18O(1-0) intensity ratios across nine nearby spiral galaxies. These isotopologues of CO…

astro-ph.GA2019

EMPIRE: The IRAM 30-m Dense Gas Survey of Nearby Galaxies

María J. Jiménez-Donaire, F. Bigiel, A. K. Leroy +14

We present EMPIRE, an IRAM 30-m large program that mapped mm dense gas tracers at kpc resolution across the whole star-forming disk of nine nearby, massiv…

astro-ph.GA2019

Dense gas is not enough: environmental variations in the star formation efficiency of dense molecular gas at 100pc scales in M51

M. Querejeta, E. Schinnerer, A. Schruba +17

It remains unclear what sets the efficiency with which molecular gas transforms into stars. Here we present a new VLA map of the spiral galaxy M51 in 33GHz radio continuum, an exti…

astro-ph.GA2016

Optical Depth Estimates and Effective Critical Densities of Dense Gas Tracers in the Inner Parts of Nearby Galaxy Discs

M. J. Jimenez-Donaire, F. Bigiel, A. K. Leroy +17

High critical density molecular lines like HCN(1-0) or HCO+(1-0) represent our best tool to study currently star-forming, dense molecular gas at extragalactic distances. The optica…

astro-ph.GA2018

Full-disc CO(1-0) mapping across nearby galaxies of the EMPIRE survey and the CO-to-H conversion factor

D. Cormier, F. Bigiel, M. J. Jiménez-Donaire +16

Carbon monoxide (CO) provides crucial information about the molecular gas properties of galaxies. While CO has been targeted extensively, isotopologues such as CO hav…