MAUNA KEA, Hawaii (November 11th, 2004) An international team led by an Edinburgh astronomer have discovered that by studying polarised light from black holes they can focus much more closely on what exactly is going on around them. The work is published this week in the monthly notices of the Royal Astronomical Society on November 11th.
Studying black holes at the centre of galaxies is difficult. A huge amount of material is falling on to the centre in an active black hole system, and this falling material is thought to power the black hole, but scientists still don’t understand this powering mechanism. One critical reason is that these black holes are just too far away for astronomers to isolate the light from them – or more accurately, the light from the compact region where the black holes are actually producing their energy.
However, Kishimoto at the University of Edinburgh and the international team of Antonucci at UC Santa Barbara, Boisson at Paris Observatory, and Blaes also at UC Santa Barbara, have used the Keck I telescope in Hawaii and European Southern Observatory’s Very Large Telescope in Chile, to do this isolation of the light. They have looked at a small part of the light emitted from black holes – light that has been scattered as it passes through the clouds very nearby. This scattered light can cleverly be picked up by looking through a polaroid filter just like the lens of polaroid sunglasses, which essentially blocks the unwanted light from elsewhere in the galaxy. The scattered light is polarised so the light waves all line up in the same direction and can pass through the Polaroid filter, but light from the surrounding area which is not polarised is excluded by the filter.
Dr Kishimoto, who leads the team, explained the importance of the new method: “For the first time we can use visible light to focus on the part of a galaxy that is very close to the black hole. We are interested in an area only about one light-day across. Until now, without using Polaroid filters, we couldn’t separate the visible light from the black hole from the light coming from a much larger region about 100 light-days across.” To put this in context, the galaxies surrounding the black holes are about 30,000 light years across.
As a result of this closer look the team have found a new signal in the observed light that can provide information about the material around a black hole. The signal, called a ‘Balmer edge’ feature, reveals properties of the material and will allow the team to carry out more detailed modelling of the temperature and density of the region near black holes than has been possible before now. This feature is commonly used to diagnose the nature of the surface of the Sun and other stars, but has never before been seen in visible light from black holes.
The next step is for Kishimoto and his team to take a look at more black holes using this technique to see if the black holes at the centre of different types of galaxy all look the same. They can then try to understand the mechanism that powers a black hole. Kishimoto and the team are now observing many other black holes using other large telescopes.
Note for editors: One light-day is the distance light travels in one day i.e. 1/365 of a light-year.