NGC 92 in H-alpha

The largest member of the galaxy group known as Robert''s Quartet is NGC 92, a spiral Sa galaxy with an unusual appearance. One of its arms, about 100,000 light-years long, has been distorted by interactions and contains a large quantity of dust. Using this H-alpha image obtained with FORS2 on the VLT, astronomers were able to study the properties of regions of active star formation ("HII regions"). They found more than 200 of such regions in NGC 92, with a size between 500 and 1,500 light-years.

Credit:

ESO

Over de afbeelding

Id:eso0535b
Type:Observatie
Publicatiedatum:4 november 2005
Gerelateerde berichten:eso0535
Grootte:1789 x 1929 px

Over het object

Naam:NGC 92, Roberts's Quartet
Type:Local Universe : Galaxy : Grouping : Cluster
Local Universe : Galaxy : Type : Spiral
Afstand:150 miljoen lichtjaren
Constellation:Phoenix
Categorie:Galaxies

Afbeeldingstypen

Grote JPEG
1,6 MB

Achtergrond

1024x768
303,7 KB
1280x1024
553,8 KB
1600x1200
882,6 KB
1920x1200
1,1 MB
2048x1536
1,4 MB

Coordinates

Position (RA):0 21 31.71
Position (Dec):-48° 37' 30.08"
Field of view:2.98 x 3.21 arcminutes
Orientation:North is 0.3° right of vertical

Kleuren & filters

BandTelescoop
Optisch
H-alpha
Very Large Telescope
FORS2