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:About the Image
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 |
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
| Band | Wavelength | Telescope |
|---|---|---|
| Optical V | 555 nm |
Hubble Space Telescope
WFPC1 |
| Optical R | 702 nm |
Hubble Space Telescope
WFPC1 |
| Infrared I | 785 nm |
Hubble Space Telescope
WFPC1 |

