Sorry! This page is not yet available in your preferred language, so we're displaying the original version instead.
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.
Crédit:ESO
À propos de l'image
Identification: | eso0535b |
Type: | Observation |
Date de publication: | 4 novembre 2005 |
Communiqués de presse en rapport: | eso0535 |
Taille: | 1789 x 1929 px |
À propos de l'objet
Nom: | NGC 92, Roberts's Quartet |
Type: | Local Universe : Galaxy : Grouping : Cluster Local Universe : Galaxy : Type : Spiral |
Distance: | 150 million années lumière |
Constellation: | Phoenix |
Catégorie: | Galaxies |
Fonds d'écran
1024x768
303,7 Kio
1280x1024
553,8 Kio
1600x1200
882,6 Kio
1920x1200
1,1 Mio
2048x1536
1,4 Mio
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 |
Couleurs & filtres
Domaine | Télescope |
---|---|
Visible H-alpha | Very Large Telescope FORS2 |