Detail of N44 in the Large Magellanic Cloud

This image of the spectacular N44 H II region in the LMC displays (very nearly) its central region, which is dominated by a large, ring-shaped nebula that includes a bright stellar association of very luminous stars. It emits X-rays - this is interpreted as a sign that several heavy stars in this area have exploded as supernova during the last few million years. N44 is a very bright, rich and well-studied complex in the LMC, somewhat apart from the other nebulae in this galaxy. The general appearance (in astronomical terminology: the "morphology") is well explained by a combination of fast outflow from stars (stellar winds) and supernova remnants, as well as sequential star formation.

Credit:

ESO

Over de afbeelding

Id:eso9931b
Type:Observatie
Publicatiedatum:22 juni 1999
Gerelateerde berichten:eso9931
Grootte:2303 x 2381 px

Over het object

Naam:N 44
Type:Local Universe : Nebula : Appearance : Emission : H II Region
Afstand:170000 lichtjaren
Constellation:Dorado
Categorie:Nebulae

Afbeeldingstypen

Grote JPEG
4,2 MB

Achtergrond

1024x768
751,7 KB
1280x1024
1,2 MB
1600x1200
1,7 MB
1920x1200
2,0 MB
2048x1536
2,6 MB

Coordinates

Position (RA):5 22 7.92
Position (Dec):-67° 56' 13.62"
Field of view:9.69 x 10.02 arcminutes
Orientation:North is 0.3° right of vertical

Kleuren & filters

BandTelescoop
Optisch
B
MPG/ESO 2.2-metre telescope
WFI
Optisch
V
MPG/ESO 2.2-metre telescope
WFI
Optisch
H-alpha
MPG/ESO 2.2-metre telescope
WFI