S315p.250 — Star Formation Rate and Gas Relations in the Arp 299 Merger from the VIXENS Survey

Date & Time

Aug 4th at 6:00 PM until 6:00 PM




Rating ( votes)

Author(s): Amanda Heiderman8, Neal J Evans7, Karl Gebhardt7, Guillermo Blanc3, Timothy Davis5, Casey Papovich4, Remco van den Bosch1, Daisuke Iono2, Min S. Yun6

Institution(s): 1. Max-Planck-Institut fur Astronomie, 2. Nobeyama Radio Observatory,, 3. Observatories of the Carnegie Institution for Science, 4. Texas A&M University, 5. University of Hertfordshire , 6. University of Massachusetts,, 7. University of Texas, 8. University of Virginia

We highlight first results from the VIRUS-P Investigation of the eXtreme ENvironments of Starbursts (VIXENS) integral field unit survey. We investigate the relationship between star formation and gas content in late interaction phase merger Arp 299 from VIXENS. By comparing Hα, Paα, and 24μm images to CO(2→1), CO(3→2), HCN(1→0), HCO+(1→0), and HI maps, we explore the relation between the star formation rate and gas surface densities on spatially resolved ~kpc scales. We find that the SFR-gas relations for Arp 299 are discrepant from known extragalactic spatially resolved relations in nearby spiral galaxies and disk-averaged relations in high-z mergers.