{"id":4,"date":"2014-08-08T18:41:37","date_gmt":"2014-08-08T18:41:37","guid":{"rendered":"http:\/\/localhost\/wordpress\/?page_id=4"},"modified":"2021-04-03T21:29:58","modified_gmt":"2021-04-03T21:29:58","slug":"my-research","status":"publish","type":"page","link":"http:\/\/localhost\/wordpress\/my-research\/","title":{"rendered":"My Research"},"content":{"rendered":"

My main research program focuses on understanding gas flows around star-forming galaxies. Indeed understanding galactic outflows and gas accretion is a key requirement for developing a complete picture of how galaxies form since both inflows of the baryons and super-nova driven outflows play a major role in regulating the gas content of galaxies, their star-formation histories and their stellar evolution. Hence, the goal<\/strong> of my research program is thus to put direct observational constraints on the cycle of baryons moving in and out of galaxies.<\/p>\n

One way to tackle this issue is to use background quasars<\/a> passing near star-forming galaxies.\u00a0 These quasars shed light on absorption lines from intervening clouds which in turn provides critical information on both the accreting of gas (inflow of fresh fuel) (Gas Fueling<\/a>) and on the galactic wind (outflows of gas ejected) phenomenon (Winds properties<\/a>).<\/p>\n

Observational projects: <\/strong>Currently, my colleagues and I are embarked on several observational projects to tackle these issues:<\/p>\n

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  1. coI: The MUSE eXtremely Deep Field (MXDF)<\/a>\n