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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
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 |
Se i WorldWide Telescope:
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 |