Early Science with the Large Millimeter Telescope: Exploring the Effect of AGN Activity on the Relationships Between Molecular Gas, Dust, and Star Formation

Abstract

The molecular gas, H${}_2$, that fuels star formation in galaxies is difficult to observe directly. As such, the ratio of $L_{\mathrm{IR}}$ to $L_{\mathrm{CO}}^{\prime }$ is an observational estimation of the star formation rate compared with the amount of molecular gas available to form stars, which is related to the star formation efficiency and the inverse of the gas consumption timescale. We test what effect an IR luminous AGN has on the ratio $L_{\mathrm{IR}}/L_{\mathrm{CO}}^{\prime }$ in a sample of 24 intermediate redshift galaxies from the 5 mJy Unbiased Spitzer Extragalactic Survey (5MUSES). We obtain new CO(1-0) observations with the Redshift Search Receiver on the Large Millimeter Telescope. We diagnose the presence and strength of an AGN using Spitzer IRS spectroscopy. We find that removing the AGN contribution to $L_{\mathrm{IR}}^{\mathrm{tot}}$ results in a mean $L_{\mathrm{IR}}^{\mathrm{SF}}/L_{\mathrm{CO}}^{\prime }$ for our entire sample consistent with the mean $L_{\mathrm{IR}}/L_{\mathrm{CO}}^{\prime }$ derived for a large sample of star forming galaxies from $z\sim 0-3$. We also include in our comparison the relative amount of polycyclic aromatic hydrocarbon emission for our sample and a literature sample of local and high redshift Ultra Luminous Infrared Galaxies and find a consistent trend between $L_{6.2}/L_{\mathrm{IR}}^{\mathrm{SF}}$ and $L_{\mathrm{IR}}^{\mathrm{SF}}/L_{\mathrm{CO}}^{\prime }$, such that small dust grain emission decreases with increasing $L_{\mathrm{IR}}^{\mathrm{SF}}/L_{\mathrm{CO}}^{\prime }$ for both local and high redshift dusty galaxies.

Accepted for publication in ApJ (to appear on December 10)

References in corpus (8)

• Cosmic Star Formation History
• Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
• COLD GASS, an IRAM legacy survey of molecular gas in massive galaxies: I. Relations between H2, HI, stellar content and structural properties
• COLD GASS, an IRAM Legacy Survey of Molecular Gas in Massive Galaxies: II. The non-universality of the Molecular Gas Depletion Timescale
• Mid-Infrared Spectral Diagnosis of Submillimeter Galaxies
• Spitzer Mid-Infrared Spectroscopy of Infrared Luminous Galaxies at z~2 II: Diagnostics
• PAH Emission from Ultraluminous Infrared Galaxies
• Dense Molecular Gas and the Role of Star Formation in the Host Galaxies of Quasi-Stellar Objects

Cited by in corpus (7)

• xCOLD GASS: the complete IRAM-30m legacy survey of molecular gas for galaxy evolution studies
• Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS): II. Cold Molecular Gas Evolution out to Redshift 6
• Dissecting Galaxies: Spatial and Spectral Separation of Emission Excited by Star Formation and AGN Activity
• The EDGE-CALIFA survey: exploring the role of the molecular gas on the galaxy star formation quenching
• CO Emission in Infrared-Selected Active Galactic Nuclei
• Star formation quenching stages of active and non-active galaxies
• A controlled study of cold dust content in galaxies from $z=0-2$