Infrared polarimetry of Mrk 231: scattering off hot dust grains in the central core
dc.creator | Lopez Rodriguez, E. | |
dc.creator | Packham, C. | |
dc.creator | Jones, T. J. | |
dc.creator | Siebenmorgen, R. | |
dc.creator | Roche, P. F. | |
dc.creator | Levenson, N. A. | |
dc.creator | Alonso Herrero, A. | |
dc.creator | Perlman, E. | |
dc.creator | Ichikawa, K. | |
dc.creator | Ramos Almeida, C. | |
dc.creator | Gonzalez Martin, O. | |
dc.creator | Nikutta, R. | |
dc.creator | Martinez Paredez, M. | |
dc.creator | Shenoy, D. | |
dc.creator | Gordon, M. S. | |
dc.creator | Telesco, C. M. | |
dc.date.accessioned | 2024-01-10T13:13:53Z | |
dc.date.accessioned | 2024-05-02T15:35:39Z | |
dc.date.available | 2024-01-10T13:13:53Z | |
dc.date.available | 2024-05-02T15:35:39Z | |
dc.date.created | 2024-01-10T13:13:53Z | |
dc.date.issued | 2017 | |
dc.identifier | 10.1093/mnras/stw2491 | |
dc.identifier | 1365-2966 | |
dc.identifier | 0035-8711 | |
dc.identifier | https://doi.org/10.1093/mnras/stw2491 | |
dc.identifier | https://repositorio.uc.cl/handle/11534/78351 | |
dc.identifier | WOS:000393647100038 | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/9264938 | |
dc.description.abstract | We present high-angular (0.17-0.35 arcsec) resolution imaging polarimetric observations of Mrk 231 in the 3.1 mu m filter using MMT-Pol on the 6.5-m MMT, and in the 8.7, 10.3, and 11.6 mu m filters using CanariCam on the 10.4-m Gran Telescopio CANARIAS. In combination with already published observations, we compile the 1-12 mu m total and polarized nuclear spectral energy distribution (SED). The total flux SED in the central 400 pc is explained as the combination of (1) a hot (731 +/- 4 K) dusty structure, directly irradiated by the central engine, which is at 1.6 +/- 0.1 pc away and attributed to be in the pc-scale polar region, (2) an optically-thick, smooth and disc-like dusty structure ('torus') with an inclination of 48 degrees +/- 23 degrees surrounding the central engine, and (3) an extinguished (A(V) = 36 +/- 5 mag) starburst component. The polarized SED decreases from 0.77 +/- 0.14 per cent at 1.2 mu m to 0.31 +/- 0.15 per cent at 11.6 mu m and follows a power-law function, lambda(similar to 0.57). The polarization angle remains constant (similar to 108 degrees) in the 1-12 mu m wavelength range. The dominant polarization mechanism is explained as scattering-off hot dust grains in the pc-scale polar regions. | |
dc.language | en | |
dc.publisher | OXFORD UNIV PRESS | |
dc.rights | registro bibliográfico | |
dc.subject | techniques: high angular resolution | |
dc.subject | techniques: polarimetric | |
dc.subject | galaxies: active | |
dc.subject | galaxies: Seyfert | |
dc.subject | infrared: galaxies | |
dc.subject | ACTIVE GALACTIC NUCLEI | |
dc.subject | SPECTRAL ENERGY-DISTRIBUTIONS | |
dc.subject | SEYFERT-GALAXIES | |
dc.subject | ULTRAVIOLET-SPECTRUM | |
dc.subject | WAVELENGTH DEPENDENCE | |
dc.subject | LINEAR-POLARIZATION | |
dc.subject | EMISSION | |
dc.subject | MARKARIAN-231 | |
dc.subject | TORUS | |
dc.subject | SPECTROSCOPY | |
dc.title | Infrared polarimetry of Mrk 231: scattering off hot dust grains in the central core | |
dc.type | artículo |