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Starburst Galaxy Showers The Universe

May 21, 2004

When a galaxy known as M82 had a near-miss with its neighbour, it set off an explosive burst of star formation that sent plumes of hot gas tens of thousands of light years into space. Now a team of UK and American astronomers has discovered that these gas clouds are like the jets from a high pressure shower head.

M82 - which astronomers call a "starburst galaxy" - is located at a distance of a bit more than 10 million light years from our own Milky Way. Dr. Linda Smith, from the Department of Physics and Astronomy, UCL, explains: "M82 shows intense star formation packed in dense star clusters. This powers plumes of hot gas that extend for tens of thousands of light years above and below the starry plane of the galaxy. This cosmic hurricane is traveling at more than a million miles an hour into intergalactic space."

Dr. Smith and her postgraduate student Mark Westmoquette, together with Jay Gallagher from the University of Wisconsin-Madison, have combined images taken with the ground-based WIYN Telescope on Kitt Peak, Arizona, and pictures from the Hubble Space Telescope in near Earth orbit. This enabled them to produce a unique view of M82. "This approach allows us to combine the strength of WIYN to measure very faint diffuse emission with the superb sharpness of Hubble to obtain a full picture of the superwind emerging from M82," says Professor Gallagher.

"Our problem was how to visualize data covering a huge range in brightness and spatial scale," explains Westmoquette. "We solved this by overlaying the sharp images from the Hubble that cover the inner part of the galaxy, where resolving key details is critical, on top of WIYN data that show the extended wind."

As a result, Dr. Smith and her colleagues can trace the outer wind back to the point in the centre of the galaxy where it is being produced, like following the cloud of smoke from a power plant back to the individual chimney that produced it. Many of the stars that are formed in the M82 starburst end their short lives with a supernova explosion. That means the winds they produce are laden with chemicals known as heavy elements. "Our goal here is to understand the structure of the wind's plumes, which are key factors in the evolution of this galaxy and the eventual pollution of nearby intergalactic space with new chemical elements," says Dr. Smith.

A HIGH RESOLUTION IMAGE IS AVALIABLE via the web or ftp:

It can be downloaded from http://www.star.ucl.ac.uk/~msw/M82_pr

ftp:// ftp.star.ucl.ac.uk, username: anonymous, password: your email address;
then type "cd pub/msw" and "get M82_WIYN_and_HST_large.tif.

University College London - UCL

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