YOU ARE HERE: Home > News & Press > News archive > News 2014 > Red stars and big bulges: how black holes shape galaxies

I want information on:

Information for:


Red stars and big bulges: how black holes shape galaxies

Last Updated on Thursday, 24 April 2014 13:31
Published on Tuesday, 22 April 2014 05:00

The universe we can see is made up of billions of galaxies, each containing anywhere from hundreds of thousands to hundreds of billions of stars. Large numbers of galaxies are elliptical in shape, red and mostly made up of old stars. Another (more familiar) type is the spiral, where arms wind out in a blue thin disc from a central red bulge. On average stars in spiral galaxies tend to be much younger than those in ellipticals.

RAS press1 Bluck smallImages of a small fraction of the galaxies analysed in the new study. The galaxies are ordered by total mass of stars (rising from bottom to top) and by 'bulge to total stellar mass' ratio (rising from left to right). Galaxies that appear redder have high values for both of these measurements, meaning that the mass of the bulge – and central black hole – determines their colour. Credit: A. Bluck. Click for a larger image

Now a group of astronomers led by Asa Bluck of the University of Victoria in Canada have found a (relatively) simple relationship between the colour of a galaxy and the size of its bulge – the more massive the bulge the redder the galaxy. The researchers publish their results in the  journal Monthly Notices of the Royal Astronomical Society, published by Oxford University Press.

Dr Bluck and his team used data from the Sloan Digital Sky Survey to group together over half a million galaxies of all different colours, shapes, and masses. They then used pattern recognition software to measure the shape of each one, to see how the proportion of red stars in a galaxy varies with its other properties.

They found that the mass in the central bulge (regardless of how big the disc surrounding it may be) is the key to knowing the colour of the whole galaxy. Above a given bulge mass, galaxies are red and have no new young stars.

Almost all galaxies have supermassive black holes at their centres. The mass of the bulge is closely related to the mass of the black hole; the more massive the black hole the more energy is released into the surrounding galaxy in the form of powerful jets and X-ray emission. This can blow away and heat up gas, stopping new stars from forming.

Dr Bluck commented: "A relatively simple result, that large galaxy bulges mean red galaxies, has profound consequences. Big bulges mean big black holes and these can put an end to star formation."


Media contact

Robert Massey
Royal Astronomical Society
Tel: +44 (0)20 7734 3307 x214
Mob: +44 (0)794 124 8035
This email address is being protected from spambots. You need JavaScript enabled to view it.

Science contact

Asa Bluck
Department of Physics and Astronomy
University of Victoria
British Columbia
Tel:  +1 250 721 8655
This email address is being protected from spambots. You need JavaScript enabled to view it.


Notes for editors

The Royal Astronomical Society (RAS), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organizes scientific meetings, publishes international research and review journals, recognizes outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 3800 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others.

Follow the RAS on Twitter via @royalastrosoc