Supermassive black holes with millions or even billions of solar-masses of material are found at the nuclei of most galaxies, including our Milky Way. A torus of dust and gas orbits around the black hole (at least according to most theories) and radiates in ultraviolet light when material falling toward the black hole heats the disk to millions of degrees. The accretion process can also power the ejection of jets of rapidly moving charged particles. Such actively accreting supermassive black holes in galaxies are called active galactic nuclei (AGN).
CfA astronomer Anna Pancoast and a team of her colleagues analyzed reverberation mapping data of four AGN to study their geometries and, in particular, the volume of hot gas known for its rapid motions, the so-called broad line region because the spectral lines have widths corresponding to as much as three thousand kilometers per second. The scientists find the geometry of this gas, at least in these four AGN, is well-described as coming from thick disks seen nearly face-on, with median radii from about 1600 AU to 4000 AU, and each with a black hole whose mass is about seventy million solar-masses (with an estimated precision for each one of about 50%). The new work was successful in modeling the observations and nearly doubles the size of the AGN sample modeled with this technique. The sample is still small, however, and more observations are being planned.
The study is published in The Astrophysical Journal.
Source: Harvard-Smithsonian Center for Astrophysics [December 30, 2017]