Nuclear molecular outflow in the Seyfert galaxy NGC 3227

ALMA observations have revealed nuclear dusty molecular disks or tori with characteristic sizes 15−40 pc in the few Seyferts and low -luminosity AGN that have been studied so far. These structures are generally decoupled both morphologically and kinematically from the host galaxy disk. We present AL...

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Bibliographic Details
Main Authors:	Alonso Herrero, A, García-Burillo, S, Pereira-Santaella, M, Davies, R, Combes, F, Vestergaard, M, Raimundo, S, Bunker, A, Díaz-Santos, T, Gandhi, P, García-Bernete, I, Hicks, E, Hönig, S, Hunt, L, Imanishi, M, Izumi, T, Levenson, N, Maciejewski1, W, Packham, C, Ramos Almeida, C, Ricci, C, Rigopoulou, D, Roche, P, Rosario, D, Schartmann, M, Usero, A, Ward, M
Format:	Journal article
Published:	EDP Sciences 2019

Nuclear molecular outflow in the Seyfert galaxy NGC 3227

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