The superwind galaxy NGC 4666

This visible light image, made with the Wide Field Imager on the MPG/ESO 2.2-metre telescope at the La Silla Observatory in Chile, shows the galaxy NGC 4666 in the centre. It 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 with neighbouring galaxies, including NGC 4668, visible to the lower left. A combination of supernova explosions and strong winds from massive stars in the starburst region drives a vast outflow of gas from the galaxy into space — a so-called “superwind”. NGC 4666 had previously been observed in X-rays by the ESA XMM-Newton space telescope, and these visible light observations were made to target background objects detected in the earlier X-ray images.

This picture, which covers a field of 16 by 12 arcminutes, is a combination of twelve CCD frames, 67 megapixels each, taken through blue, green and red filters.

Kilde:

ESO/J. Dietrich

Om billedet

Id:eso1036a
Type:Observation
Udgivelsesdato:1. september 2010 12:00
Relaterede pressemeddelelser:eso1036
Størrelse:3946 x 3168 px

Om objektet

Navn:NGC 4666
Type:Local Universe : Galaxy : Activity : Starburst
Afstand:80 million lysår
Constellation:Virgo
Kategori:Galaxies

Billedformater

Stor JPEG
4,7 MB
Skrærm JPEG
130,7 KB

Zoombar


Baggrundsbilleder

1024x768
159,3 KB
1280x1024
263,0 KB
1600x1200
404,9 KB
1920x1200
534,1 KB
2048x1536
757,1 KB

Koordinater

Position (RA):12 45 8.68
Position (Dec):0° 27' 43.36"
Field of view:15.64 x 12.55 arcminutes
Orientering:Nord er 0.0° droite fra lodret

Farver & filtre

BåndBølgelængdeTeleskop
Optisk
B
451 nmMPG/ESO 2.2-metre telescope
WFI
Optisk
V
539 nmMPG/ESO 2.2-metre telescope
WFI
Optisk
R
651 nmMPG/ESO 2.2-metre telescope
WFI