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We report on the coexistence of powerful gas outflows observed in millimeterand X-ray data of the Radio-Loud Narrow Line Seyfert 1 Galaxy IRAS 17020+4544.Thanks to the large collecting power of the Large Millimeter Telescope, aprominent line arising from the 12CO(1-0) transition was revealed in recentobservations of this source. The complex profile is composed by a narrowdouble-peak line and a broad wing. While the double-peak structure may bearising in a disk of molecular material, the broad wing is interpreted as thesignature of a massive outflow of molecular gas with an approximate bulkvelocity of -660 km/s. This molecular wind is likely associated to amulti-component X-ray Ultra-Fast Outflow with velocities reaching up to ~0.1cand column densities in the range 10^{21-23.9} cm^-2 that was reported in thesource prior to the LMT observations. The momentum load estimated in the twogas phases indicates that within the observational uncertainties the outflow isconsistent with being propagating through the galaxy and sweeping up the gaswhile conserving its energy. This scenario, which has been often postulated asa viable mechanism of how AGN feedback takes place, has so far been observedonly in ULIRGs sources. IRAS 17020+4544 with bolometric and infrared luminosityrespectively of 5X10^{44} erg/s and 1.05X10^{11} L_sun appears to be an exampleof AGN feedback in a NLSy1 Galaxy (a low power AGN). New proprietarymulti-wavelength data recently obtained on this source will allow us tocorroborate the proposed hypothesis.

the astrophysical journal. letters

Early Science with the Large Millimeter Telescope: an energy-driven wind  revealed by massive molecular and fast X-ray outflows in the Seyfert Galaxy  IRAS 17020+4544