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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.
Källa:ESO
Om bilden
ID: | eso0437e |
Typ: | Observation |
Publiceringsdatum: | 10 december 2004 |
Relaterade pressmeddelanden: | eso0437 |
Storlek: | 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 är 1.0° höger om lodrätt |
Färger och filter
Band | Teleskop |
---|---|
Ultraviolett U | MPG/ESO 2.2-metre telescope WFI |
Synligt ljus Oiii | MPG/ESO 2.2-metre telescope WFI |
Synligt ljus H-alpha | MPG/ESO 2.2-metre telescope WFI |