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N44 in the Large Magellanic Cloud
This image of the spectacular N44 H II region in the LMC displays (very nearly) the full extent of the WFI field. 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.
Kilde:ESO
Om billedet
Id: | eso9931a |
Type: | Observation |
Udgivelsesdato: | 22. juni 1999 |
Relaterede pressemeddelelser: | eso9931 |
Størrelse: | 2303 x 2229 px |
Om objektet
Navn: | N 44 |
Type: | Local Universe : Nebula : Appearance : Emission : H II Region |
Afstand: | 170000 lysår |
Constellation: | Dorado |
Kategori: | Nebulae |
Baggrundsbilleder
1024x768
854,1 KB
1280x1024
1,4 MB
1600x1200
1,9 MB
1920x1200
2,1 MB
2048x1536
2,8 MB
Koordinater
Position (RA): | 5 21 37.89 |
Position (Dec): | -67° 54' 42.77" |
Field of view: | 31.47 x 30.46 arcminutes |
Orientering: | Nord er 0.4° droite fra lodret |
Farver & filtre
Bånd | Teleskop |
---|---|
Optisk B | MPG/ESO 2.2-metre telescope WFI |
Optisk V | MPG/ESO 2.2-metre telescope WFI |
Optisk H-alpha | MPG/ESO 2.2-metre telescope WFI |