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.

Källa:

ESO/J. Dietrich

Om bilden

ID:eso1036a
Typ:Observation
Publiceringsdatum:1 september 2010 12:00
Relaterade pressmeddelanden:eso1036
Storlek:3946 x 3168 px

Om objektet

Namn:NGC 4666
Typ:Local Universe : Galaxy : Activity : Starburst
Avstånd:80 miljon ljusår
Constellation:Virgo
Kategori:Galaxies

Bildformat

Originalstorlek
30,4 MB
Stor jpeg
4,7 MB
Skärmstor jpeg
130,7 kB

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Skrivbordsunderlägg

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 är 0.0° höger om lodrätt

Färger och filter

BandVåglängdTeleskop
Synligt ljus
B
451 nmMPG/ESO 2.2-metre telescope
WFI
Synligt ljus
V
539 nmMPG/ESO 2.2-metre telescope
WFI
Synligt ljus
R
651 nmMPG/ESO 2.2-metre telescope
WFI