The superwind galaxy NGC 4666 (w/ Video)

The prominent galaxy NGC 4666 in the centre of the picture is a starburst galaxy, about 80 million light-years from Earth, in which particularly intense star formation is taking place. The starburst is thought to be caused by gravitational interactions between NGC 4666 and its neighbouring galaxies, including NGC 4668, visible to the lower left. These interactions often spark vigorous star-formation in the galaxies involved.

A combination of supernova explosions and strong winds from massive stars in the starburst region drives a vast flow of gas from the galaxy into space — a so-called "superwind". The superwind is huge in scale, coming from the bright central region of the galaxy and extending for tens of thousands of light-years. As the superwind gas is very hot it emits radiation mostly as X-rays and in the radio part of the spectrum and cannot be seen in visible light images such as the one presented here.

This image was made as part of a follow-up to observations made with the ESA XMM-Newton space telescope in X-rays. NGC 4666 was the target of the original XMM-Newton observations, but thanks to the telescope's wide field-of-view many other X-ray sources were also seen in the background. One such serendipitous detection is a faint galaxy cluster seen close to the bottom edge of the image, right of centre. This cluster is much further away from us than NGC 4666, at a distance of about three billion light-years.

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In this zoom sequence we start with a view of part of the constellation of Virgo, far from the plane of the Milky Way and home to the Virgo cluster of galaxies. The brilliant double star Gamma Virginis appears at the lower right and we can faintly see the galaxy NGC 4666 above the centre of the picture. This apparently insignificant oval is in fact a starburst galaxy, about 80 million light-years from Earth, in which particularly intense star formation is taking place. The final part of the sequence shows the detailed Wide Field Imager view of the galaxy and its environment. Credit: ESO/J. Dietrich, Digitized Sky Survey 2. Acknowledgment: Davide De Martin. Music: John Dyson (from the album "Darklight")

In order to fully understand the nature of astronomical objects, researchers must study them at several wavelengths. This is because light of different wavelengths can tell us about different physical processes taking place. In this case the Wide Field Imager (WFI) observations were made in visible light to further investigate these serendipitously detected X-ray objects — a good example of how astronomers using different telescopes work together to explore the Universe.

More information: Science paper: A&A 449, 837

Provided by ESO (news : web)