Examinando por Autor "Longinotti, A. L."

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MUSE Reveals Extended Circumnuclear Outflows in the Seyfert 1 NGC 7469
(IOP Science Publishing, 2021-01-11) Robleto Orús, A. C.; Torres Papaqui, J. P.; Longinotti, A. L.; Ortega Minakata, R. A.; Sánchez, S. F.; Ascasibar, Y.; Bellocchi, E.; Galbany, L.; Chow Martínez, M.; Trejo Alonso, J. J.; Morales Vargas, A.; Romero Cruz, F. J.; Consejo Nacional de Ciencia y Tecnología (CONACYT); Agencia Estatal de Investigación (AEI); European Research Council (ERC); Comunidad de Madrid; Robleto Orús, A. C. [0000-0002-4216-7138]; Torres Papaqui, J. P. [0000-0002-8009-0637]; Longionotti, A. L. [0000-0001-8825-3624]; Ortega Minakata, R. A. [0000-0002-8322-6333]; Sánchez, S. F. [0000-0001-6444-9307]; Ascasibar, Y. [0000-0003-1577-2479]; Bellocchi, E. [0000-0001-9791-4228]; Galbany, L. [0000-0002-1296-6887]; Chow Martínez, M. [0000-0001-6073-9956]; Trejo Alonso, J. J. [0000-0003-2293-1802]; Morales Varga, A. [0000-0002-9137-861X]; Romero Cruz, F. J. [0000-0003-0962-8390]; Unidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737
NGC 7469 is a well-known luminous infrared galaxy, with a circumnuclear star formation ring (∼830 pc radius) surrounding a Seyfert 1 active galactic nucleus (AGN). Nuclear unresolved winds were previously detected in X-rays and ultraviolet, as well as an extended biconical outflow in infrared coronal lines. We search for extended outflows by measuring the kinematics of the Hβ and [O iii] λ5007 optical emission lines, in data of the Very Large Telescope/Multi-unit Spectroscopic Explorer integral field spectrograph. We find evidence of two outflow kinematic regimes: one slower regime extending across most of the star formation (SF) ring—possibly driven by the massive SF—and a faster regime (with a maximum velocity of −715 km s−1), only observed in [O iii], in the western region between the AGN and the massive star-forming regions of the ring, likely AGN-driven. This work shows a case where combined AGN/SF feedback can be effectively spatially resolved, opening up a promising path toward a deeper understanding of feedback processes in the central kiloparsec of AGN.