Modeling the Unresolved NIR-MIR SEDs of Local (z < 0.1) QSOs
To study the nuclear (≲1 kpc) dust of nearby (z < 0.1) quasi-stellar objects (QSOs), we obtained new near-infrared (NIR) high angular resolution (~0.″3) photometry in the H and Ks bands for 13 QSOs with available mid-infrared (MIR) high angular resolution spectroscopy (~7.5-13.5 μm). We find that in most QSOs, the NIR emission is unresolved. We
Martínez-Paredes, M. et al.
Fecha de publicación:
12
2021