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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.
Kredit:ESO
O snímku
Id: | eso0437e |
Typ: | Pozorování |
Datum zveřejnění: | 10. prosince 2004 |
Související články: | eso0437 |
Velikost: | 1744 x 1644 px |
O objektu
Jméno: | N 164 |
Typ: | Local Universe : Nebula |
Vzdálenost: | 170000 světelné roky |
Constellation: | Dorado |
Kategorie: | Nebulae |
Souřadnice
Position (RA): | 5 38 42.61 |
Position (Dec): | -69° 6' 3.89" |
Field of view: | 6.93 x 6.53 arcminutes |
Orientace: | Sever je 1.0° pravá od svislé osy |
Barvy & filtry
Pásmo | Dalekohled |
---|---|
Ultrafialový U | MPG/ESO 2.2-metre telescope WFI |
Optický Oiii | MPG/ESO 2.2-metre telescope WFI |
Optický H-alpha | MPG/ESO 2.2-metre telescope WFI |