HST planetary camera images of core of peculiar galaxy Arp 220

An image of the central part of the ultra-luminuous infrared galaxy Arp 220 taken with the WFPC on the Hubble Space Telescope. HST reveals a new complex structure within one arc second of the nucleus. While part of the this structure was seen in radio interfero-metric maps, most of the structure is new.

HST reveals a new class of object at the core: gigantic young star clusters which are ten times larger than any clusters observed previously. They were probably produces by the collision of two spiral galaxies. Stars are produced at a furious rate from the dust and gas supplied by the collision.

Credit:

E. Shaya, D. Dowling/U. of Maryland, the WFPC Team, and NASA/ESA

About the Image

NASA press release
Id:opo9216b
Type:Observation
Release date:2 June 1992, 06:00
Size:2863 x 2408 px

About the Object

Name:Arp 220
Type:Local Universe : Galaxy : Type : Irregular
Local Universe : Galaxy : Component : Center/Core
Distance:250 million light years
Constellation:Serpens Caput
Category:Galaxies

Image Formats

r.titleLarge JPEG
2.1 MB
r.titleScreensize JPEG
239.4 KB

Coordinates

Position (RA):15 34 57.37
Position (Dec):23° 30' 11.09"
Field of view:0.32 x 0.27 arcminutes
Orientation:North is 6.9° right of vertical


Colours & filters

BandWavelengthTelescope
Optical
V
555 nm Hubble Space Telescope
WFPC1
Optical
R
702 nm Hubble Space Telescope
WFPC1
Infrared
I
785 nm Hubble Space Telescope
WFPC1

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