Artigo Acesso aberto Revisado por pares

Superbubble in the Large Magellanic Cloud

2011; Oxford University Press; Volume: 52; Issue: 5 Linguagem: Inglês

10.1111/j.1468-4004.2011.52504_3.x

ISSN

1468-4004

Tópico(s)

Planetary Science and Exploration

Resumo

Superbubble in the Large Magellanic CloudSuperbubble LHA 120-N 44 in NGC1929, part of the Large Magellanic Cloud, is formed by the stellar winds from hot young stars -blue/white in this image -shaping the clouds of gas and dust, in this image from the European Southern Observatory.Shockwaves from supernova explosions add to the effect, and the intense ultraviolet radiation from the stars makes the gas and dust glow.As the gas and dust is compressed, new stars form in turn.This close-up image was made from ESO Very Large Telescope FORS-1 images identified by Manu Mejias, from Argentina, in ESO's 2010 Hidden Treasures competition, in which people were invited to find impressive images in ESO archives.(ESO/Manu Mejias)

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