Keck OSIRIS AO LIRG Analysis: Feedback in the Nuclei of Luminous Infrared Galaxies
| Autor: | U, Vivian, Medling, Anne M., Inami, Hanae, Armus, Lee, Díaz-Santos, Tanio, Charmandaris, Vassilis, Howell, Justin, Stierwalt, Sabrina, Privon, George C., Linden, Sean T., Sanders, David B., Max, Claire E., Evans, Aaron S., Barcos-Muñoz, Loreto, Chiang, Charleston W. K., Appleton, Phil, Canalizo, Gabriela, Fazio, Giovanni, Iwasawa, Kazushi, Larson, Kirsten, Mazzarella, Joseph, Murphy, Eric, Rich, Jeffrey, Surace, Jason |
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| Rok vydání: | 2018 |
| Předmět: | |
| Zdroj: | 2019 ApJ, 871, 166 |
| Druh dokumentu: | Working Paper |
| DOI: | 10.3847/1538-4357/aaf1c2 |
| Popis: | The role of feedback in triggering or quenching star formation and hence driving galaxy evolution can be directly studied with high resolution integral field observations. The manifestation of feedback in shocks is particularly important to examine in galaxy mergers, where violent interactions of gas takes place in the interstellar medium during the course of the galactic collision. As part of our effort to systematically study the local population of luminous infrared galaxies within the Great Observatories All-Sky LIRG Survey, we undertook the Keck OSIRIS AO LIRG Analysis observing campaign to study the gas dynamics in the inner kiloparsec regions of these systems at spatial scales of a few 10s of parsecs. With high-resolution near-infrared adaptive optics-assisted integral-field observations taken with OSIRIS on the Keck Telescopes, we employ near-infrared diagnostics such as Brg and the ro-vibrationally excited H2 lines to quantify the nuclear star formation rate and identify feedback associated with shocked molecular gas seen in 21 nearby luminous infrared galaxies. Shocked molecular gas is preferentially found in the ultraluminous infrared systems, but may also be triggered at a lower luminosity, earlier merging stage. On circumnuclear scales, AGN have a strong effect on heating the surrounding molecular gas, though their coupling is not simply driven by AGN strength but rather is complicated by orientation, dust shielding, density, and other factors. We find that the nuclear star formation correlates with merger class and diminishing projected nuclear separations. These trends are largely consistent with the picture of merger-induced starbursts within the center of galaxy mergers. Comment: Accepted to ApJ; 31 pages (with 5 tables and 10 embedded figures) + figure set |
| Databáze: | arXiv |
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