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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.
Crédit:ESO
À propos de l'image
Identification: | eso0437e |
Type: | Observation |
Date de publication: | 10 décembre 2004 |
Communiqués de presse en rapport: | eso0437 |
Taille: | 1744 x 1644 px |
À propos de l'objet
Nom: | N 164 |
Type: | Local Universe : Nebula |
Distance: | 170000 années lumière |
Constellation: | Dorado |
Catégorie: | Nebulae |
Fonds d'écran
1024x768
366,8 Kio
1280x1024
579,7 Kio
1600x1200
833,2 Kio
1920x1200
944,5 Kio
2048x1536
1,3 Mio
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 |
Couleurs & filtres
Domaine | Télescope |
---|---|
Ultraviolet U | MPG/ESO 2.2-metre telescope WFI |
Visible Oiii | MPG/ESO 2.2-metre telescope WFI |
Visible H-alpha | MPG/ESO 2.2-metre telescope WFI |