Optical Detection of the Hidden Nuclear Engine in NGC~4258
arXiv:astro-ph/9510006 · doi:10.1086/309817
Abstract
The sub-parsec masing disk recently found to be orbiting a central mass of ~\msun\ in the Seyfert/LINER galaxy NGC~4258 provides the most compelling evidence to date for the existence of a massive black hole in the nucleus of a galaxy. The disk is oriented nearly edge-on %(°) and the X-ray spectrum %(Makishima \etal\ 1994) is heavily absorbed. Therefore, in this galaxy, the optical emission-line spectrum generally exhibited by an active galactic nucleus is perhaps best sought using polarized light: probing for light scattered off material surrounding the central source. New polarimetry of NGC~4258 has uncovered a compact polarized nucleus whose spectrum consists of a faint blue continuum similar to those of unobscured quasars (), plus broadened (\twid1000\kms) emission lines. The lines are strongly linearly polarized (\%) at a position angle (85°2°) coincident with the plane of the maser disk. This result provides substantiating evidence for a weakly active central engine in NGC~4258 and for the existence of obscuring, orbiting tori which impart many of the perceived distinctions between various types of active galaxy.
Accepted by ApJ Letters, 16 pages including 3 figures; uuencoded, gzipped postscript, also available via anon ftp at ftp://head-cfa.harvard.edu/pub/transfer/belinda/ngc4258_apjl.ps
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