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.

Kredit:

ESO

O snímku

Id:eso9931b
Typ:Pozorování
Datum zveřejnění:22. června 1999
Související články:eso9931
Velikost:2303 x 2381 px

O objektu

Jméno:N 44
Typ:Local Universe : Nebula : Appearance : Emission : H II Region
Vzdálenost:170000 světelné roky
Constellation:Dorado
Kategorie:Nebulae

Image Formats


Pozadí

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

Souřadnice

Position (RA):5 22 7.92
Position (Dec):-67° 56' 13.62"
Field of view:9.69 x 10.02 arcminutes
Orientace:Sever je 0.3° pravá od svislé osy

Barvy & filtry

PásmoDalekohled
Optický
B
MPG/ESO 2.2-metre telescope
WFI
Optický
V
MPG/ESO 2.2-metre telescope
WFI
Optický
H-alpha
MPG/ESO 2.2-metre telescope
WFI