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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.
Credit:ESO
Over de afbeelding
Id: | eso0437e |
Type: | Observatie |
Publicatiedatum: | 10 december 2004 |
Gerelateerde berichten: | eso0437 |
Grootte: | 1744 x 1644 px |
Over het object
Naam: | N 164 |
Type: | Local Universe : Nebula |
Afstand: | 170000 lichtjaren |
Constellation: | Dorado |
Categorie: | Nebulae |
Achtergrond
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Coordinates
Position (RA): | 5 38 42.61 |
Position (Dec): | -69° 6' 3.89" |
Field of view: | 6.93 x 6.53 arcminutes |
Orientation: | North is 1.0° right of vertical |
Kleuren & filters
Band | Telescoop |
---|---|
Ultraviolet U | MPG/ESO 2.2-metre telescope WFI |
Optisch Oiii | MPG/ESO 2.2-metre telescope WFI |
Optisch H-alpha | MPG/ESO 2.2-metre telescope WFI |