Discovery of an Active Galactic Nucleus Driven Molecular Outflow in the Local Early-type Galaxy NGC 1266

Alatalo, K.; Blitz, L.; Young, L. M.; Davis, T. A.; Bureau, M.; Lopez, L. A.; Cappellari, M.; Scott, N.; Shapiro, K. L.; Crocker, A. F.; Martín, S.; Bois, M.; Bournaud, F.; Davies, R. L.; de Zeeuw, P. T.; Duc, P.-A.; Emsellem, E.; Falcón-Barroso, J.; Khochfar, S.; Krajnović, D.; Kuntschner, H.; Lablanche, P.-Y.; McDermid, R. M.; Morganti, R.; Naab, T.; Oosterloo, T.; Sarzi, M.; Serra, P.; Weijmans, A.
Referencia bibliográfica

The Astrophysical Journal, Volume 735, Issue 2, article id. 88 (2011).

Fecha de publicación:
7
2011
Número de autores
29
Número de autores del IAC
1
Número de citas
267
Número de citas referidas
237
Descripción
We report the discovery of a powerful molecular wind from the nucleus of the non-interacting nearby S0 field galaxy NGC 1266. The single-dish CO profile exhibits emission to ±400 km s-1 and requires a nested Gaussian fit to be properly described. Interferometric observations reveal a massive, centrally concentrated molecular component with a mass of 1.1 × 109 M sun and a molecular outflow with a molecular mass of ≈2.4 × 107 M sun. The molecular gas close to the systemic velocity consists of a rotating, compact nucleus with a mass of about 4.1 × 108 M sun within a radius of ≈60 pc. This compact molecular nucleus has a surface density of ≈2.7 × 104 M sun pc-2, more than two orders of magnitude larger than that of giant molecular clouds in the disk of the Milky Way, and it appears to sit on the Kennicutt-Schmidt relation despite its extreme kinematics and energetic activity. We interpret this nucleus as a disk that confines the outflowing wind. A mass outflow rate of ≈13 M sun yr-1 leads to a depletion timescale of lsim85 Myr. The star formation in NGC 1266 is insufficient to drive the outflow, and thus it is likely driven by the active galactic nucleus. The concentration of the majority of the molecular gas in the central 100 pc requires an extraordinary loss of angular momentum, but no obvious companion or interacting galaxy is present to enable the transfer. NGC 1266 is the first known outflowing molecular system that does not show any evidence of a recent interaction.
Proyectos relacionados
Miembros del grupo
Huellas de la Formación de las Galaxias: Poblaciones estelares, Dinámica y Morfología
Bienvenida a la página web del g rupo de investigación Traces of Galaxy Formation. Somos un grupo de investigación amplio, diverso y muy activo cuyo objetivo principal es entender la formación de galaxias en el Universo de una manera lo más completa posible. Con el estudio detellado de las poblaciones estelares como bandera, estamos constantemente
Ignacio
Martín Navarro