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LHA 120-N 55 is an emission nebula located within the Large Magellanic Cloud (LMC). It is a glowing clump of gas and dust that gets its light output from the hydrogen atoms shedding electrons within it. It was named in 1956, in a catalogue of H-alpha emission line objects in the LMC. Multiple dense molecular clumps have been detected, at least fifteen of which contain young stellar objects.

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  • LHA 120-N 55 (en)
  • LHA 120-N 55 (nl)
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  • LHA 120-N 55 is an emission nebula located within the Large Magellanic Cloud (LMC). It is a glowing clump of gas and dust that gets its light output from the hydrogen atoms shedding electrons within it. It was named in 1956, in a catalogue of H-alpha emission line objects in the LMC. Multiple dense molecular clumps have been detected, at least fifteen of which contain young stellar objects. (en)
  • LHA 120-N 55 is een emissienevel in de Grote Magelhaense Wolk (GMW). Het is een gloeiende wolk gas en stof die zijn lichtopbrengst krijgt door de ionisatie van waterstofatomen. Hij kreeg zijn naam in 1956, in een catalogus van H-alfa emissielijnobjecten in de GMW. Er zijn meerdere dichte moleculaire wolken gedetecteerd, waarvan er ten minste vijftien jonge stellaire objecten bevatten. (nl)
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  • LHA 120-N 55 (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/The_glowing_gas_cloud_LHA_120-N55_in_the_Large_Magellanic_Cloud.jpg
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  • VLT image of LHA 120-N 55 (en)
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  • DEM L 228 (en)
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  • nebula (en)
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  • LHA 120-N 55 is an emission nebula located within the Large Magellanic Cloud (LMC). It is a glowing clump of gas and dust that gets its light output from the hydrogen atoms shedding electrons within it. It was named in 1956, in a catalogue of H-alpha emission line objects in the LMC. Multiple dense molecular clumps have been detected, at least fifteen of which contain young stellar objects. (en)
  • LHA 120-N 55 is een emissienevel in de Grote Magelhaense Wolk (GMW). Het is een gloeiende wolk gas en stof die zijn lichtopbrengst krijgt door de ionisatie van waterstofatomen. Hij kreeg zijn naam in 1956, in een catalogus van H-alfa emissielijnobjecten in de GMW. Er zijn meerdere dichte moleculaire wolken gedetecteerd, waarvan er ten minste vijftien jonge stellaire objecten bevatten. (nl)
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  • ESO (en)
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