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N 164 nebula in the LMC
N 164, a bright nebula, the glow of which is caused by hot stars inside it. The heating of the gas by these stars increases the pressure and causes such nebulae to expand, pushing outwards against their surroundings. A careful look at this nebula reveals locations where the expansion is encountering resistance by denser clouds of gas, producing bright, thin rims. The sky field measures 3.6 x 3.5 arcmin. North is up and East is left.
Kilde:ESO
Om billedet
Id: | eso0437e |
Type: | Observation |
Udgivelsesdato: | 10. december 2004 |
Relaterede pressemeddelelser: | eso0437 |
Størrelse: | 1744 x 1644 px |
Om objektet
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Koordinater
Position (RA): | 5 38 42.61 |
Position (Dec): | -69° 6' 3.89" |
Field of view: | 6.93 x 6.53 arcminutes |
Orientering: | Nord er 1.0° droite fra lodret |
Farver & filtre
Bånd | Teleskop |
---|---|
Ultraviolet U | MPG/ESO 2.2-metre telescope WFI |
Optisk Oiii | MPG/ESO 2.2-metre telescope WFI |
Optisk H-alpha | MPG/ESO 2.2-metre telescope WFI |